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A A Vy ill 1 ilk. j! ill! iilli'l j iSpi ill ' \V -w »T«t X.' C'r‘ 1 yP£^'^ >» %;f-Ao&V4X#/' i-XfL %, %S5if® H,fir, %. wM&$y A v^‘ J&* Xh k-o y /m X. > £,,« yop3 > \v'4 &-.j~'k--$ ml ‘A .'k '^Ty a _ ~y X> ^d» S' s.Xx sr _ v > 4 O, i BSXXi liEl] \l’-3L7^A- i ■’££'$ f/ Uyt I'jA •■■ y{ A* ?/ \% O b-/Om-j. i t &■&>// $>' A 4/ v **:¥ % I V \0 A‘‘ „v IMSU t XSp wA A 44S'J /> ninth „ ,, “+1*20,” „ “-1*30.’ 5) PROCEEDINGS OF THE ROYAL SOCIETY OF EDINBURGH. VOL. IX. 1875-76. No. 93. Ninety-Third Session. Monday , 22 d November 1875. Sir ROBERT CHRISTISON, Bart., Hon. Vice-President, in the Chair. The foRowing Council were elected :■ — President. Sir WILLIAM THOMSON, Knt., LL.D. Honorary Vice-Presidents. His Grace the DUKE of ARGYLL. Sir ROBERT CHRISTISON, Bart., M.D. Vice-Presidents. David Milne Home, LL.D. Professor Kelland. Rev.W. Lindsay Alexander, D.D. David Stevenson, Esq., C.E. The Hon Lord Neaves. The Right Rev. Bishop Cotthrill. General Secretary — Dr John Hutton Balfour. Secretaries to Ordinary Meetings. Professor Tait. Professor Turner. Treasurer-— David Smith, Esq. Curator of Library and Museum — Dr Maclaoan. Councillors. Dr Arthur Mitchell. George Forbes, Esq. Principal Sir Alex. Grant, Bart. Professor Geikie. Dr Andrew Fleming, H.M.I.S. Dr Charles Moreread. Alexander Buchan, A.M. Robert Wyld, Esq. Dr Ramsay H. Traquair. Dr Thomas Harvey. Dr John G. M‘Kendrick. Dr J. Matthews Duncan. vol. IX. A 2 Proceedings of the Royal Society Monday, §th December 1875. DAVID MILNE HOME, Esq., of Wedderburn, LL.D., Senior Vice-President, in the Chair. The Chairman delivered the following opening Address: — Gentlemen, Fellows of the Royal Society of Edinburgh, — In compliance with a request of the Council, I have the honour to come before you this evening to give an address, on this the first night of our Winter Session, in pursuance of the custom prevalent in this and most other Societies. I need not say how much 1 regret, for your sakes as well as my own, that this duty is not to be discharged by our eminent Presi- dent. The first point which I will submit to your notice, is the nature and amount of the work we as a Society are doing, and our means of doing it. The second and concluding part of my Address will have reference to the present aspect and prospects of science generally ip the country. With regard to the work we are carrying on, it may be suffi- cient to refer to the proceedings of our last winter’s session. Our Secretary tells me that it was the longest session he remembers — it having been prolonged beyond mid-summer. You are aware that our Society was intended by its founders to embrace literature as well as science ; and that in regard to science, we encourage investigations in any of nature’s various fields. The following abstract, under different heads, of the papers read during last session, indicates the range and variety of the Society’s operations : — In Applied Mathematics or Physics, we had 11 papers read; in Pure Mathematics, 9 ; Notes from Professor Tait’s Physical Labo- ratory were read at five meetings ; of Geological papers, 4 were read ; of Chemical papers, 3 ; of Physiological papers, 3 ; of Anatomi- cal papers, 3 ; of Meteorological papers, 2 ; of Literary papers, 2 ; separate Biographical Memoirs of eleven deceased Members were of Edinburgh, Session 1875-76. 3 read. Many interesting experiments were shown at our meetings; and in particular, our President, at one of our meetings, exhibited and explained his wonderful tide-calculating machine, by means of which there can be obtained in a few seconds, results which hitherto have required minute and laborious calculations. The three Prizes which the Society has at its disposal, were awarded as follows : — The Keith Prize was awarded to Professor Tait, for his paper on a “ First Approximation to a Thermo-Electric Diagram.” The Makdougall Brisbane Prize was awarded to Professor Lister, for his paper u0n the Germ Theory of Putrefaction and Fermenta- tion.” The Neill Prize was awarded to Mr Charles William Peach, for A his “ Contributions to Scotch Geology and Zoology.” Gentlemen, an important part of our work as a Society is to publish in a volume of Transactions the most deserving of the papers read at our meetings. A copy of these Transactions is, as you know, obtained gratis by every member. Copies also, to tbe extent of considerably above a hundred, go to foreign libraries, foreign universities, and foreign societies. Many of these papers are necessarily not of so popular a character as to pay, by the sale of them, the cost of printing. But these papers, though not interesting to the general community, may be of the highest importance for the advancement of science. Fortunately our Society is sufficiently wealthy to be able to defray the expense, not only of printing, but of a large gratuitous circulation. X believe that it is a knowledge of this fact which obtains for our Society so large a membership, and so satisfactory a revenue. With regard to our membership, we have now 358 Ordinary Fellows. X observe from the address which I had the honour of giving five years ago, that the number then was 326, so that there has been in the interval an increase of 32 members. The number of members whom we have lost by death is, I am sorry to say, larger than usual, being altogether 14. The follow- ing are the names alphabetically arranged : — 4 Proceedings of the Royal Society 1 . Foreign Honorary Fellow. — Le Comte de Remusat. 2. British Honorary Fellows. — Sir Charles Lyell, Bart, of Kinnordy; Sir William Edmund Logan, LL.D.; Sir Charles Wheatstone, D.C.L. 3. Ordinary Fellows. — Rev. Dr D. Aitken ; John Auld, Esq. ; Professor Hughes Bennett, Edinburgh University; Rev. Professor Crawford, Edinburgh University; Colonel Seton Guthrie, Thurso ; Sir William Jardine of Applegarth, Bart. ; Professor William Macdonald, St Andrews’ University; the Hon. Lord Mackenzie; Edward Meldrum, Esq., Dechmont; the Venerable Archdeacon Sinclair. I propose to give an obituary notice of several in this list, with regard to whom I have succeeded in obtaining information, chiefly through the good offices of our Secretary, Professor Balfour. Charles, Comte de Remusat, a distinguished French poli- tician, philosopher, and man of letters, was horn at Paris on the 14th of March 1797. His father held various public offices under the first Empire. His mother was an intimate friend of the Empress Josephine. The young Remusat, after a brilliant course at the Lyc6e Napoleon, betook himself at first to the study of law, but he soon turned to literature, and wrote as a journalist in newspapers and reviews from 1818 till 1830. In company with Guizot, Cousin, and Jouffroy, he was on the staff of the “ Globe,” a periodical founded by Dubois in 1824, which struggled against the growing absolutism of the Restoration. He continued afterwards, in concert with Guizot, to support doc- trinaire constitutionalism, and in philosophy he was on the whole of the school of Cousin. His name appears in the list of journalists who protested against the ordinances which brought about the Revolution of July. In 1830, he was chosen deputy by Toulouse, and soon followed the leadership of Thiers in the Chamber. In 1838, he was for a short time Under-Secretary of State in the ministry of Count Mole, and in 1840 he was Minister of the Interior, under Thiers. After the Revolution of 1848, he continued a member of the Constituent Assembly, and supported the party of order. During the whole period of the second Empire, he withdrew of Edinburgh, Session 1875-76. 5 from political life, and devoted himself to literary and philosophical labours, sceptical of the possibility of an Imperial government restoring liberal institutions. The Revolution of 1870 brought the Count de Remusat back to public life, as Minister of Foreign Affairs under M. Thiers, with whom he fell in May 1873, and with whom he agreed in regarding the Republic as, if not the political ideal, at least the best practical solution of the difficulties of France. He died at Paris on the 6th of June 1875. The Count de Remusat was a copious, solid, and eloquent writer. Besides his large contributions to the periodical press, especially the “Revue des Deux Mondes,” he was the author of many valuable works. One of his earliest essays was connected with his legal studies, and appeared in 1820 (“ Sur la procedure en Matiere Crimi- nelle ”), followed by other tracts on the responsibility of ministers of State, the liberty of the press, and the law of elections. His most brilliant and productive period as a writer was after 1840. Among his other works are the following : — Essai sur la nature de Pouvoir, 1840. Essais de Philosophie, 1842. Abelard, .... 1845. Melanges Philosophiques, . 1847. St Anselm, 1852. Bacon— Sa Vie, son Temps, 1858. La Philosophie Religieuse, . 1864. David Hartley, 1874. Philosophie Anglaise — Bacon jusqu’a Locke, 1875. As may be inferred from the subjects of his studies, M. de Remusat was deeply interested in England. Probably no eminent Frenchman of his time unders ood English institutions and national character so well. The practical philosophers and states- men of this country, and their readiness to accept the teaching of experience and to recognise the tendencies of the age, in a spirit of wise compromise, were all in harmony with his temper; which always inclined to moderation, and was averse to fanaticism, whether political or speculative, religious or anti-religious. In philosophy, he belonged to the school opposed to Materialism. In M. de Remusat we have lost one of the most eminent of the 6 Proceedings of the Royal Society French politicians and thoughtful men of letters of the nineteenth century, and the philosophy of mind has lost one of its ablest expositors, though he may not have ranked among its discoverers and leaders. Charles Lyell was born at Kinnordy, in Forfarshire, on 14th November 1797, and died in London 22d February 1875. He was on our list of British Honorary Fellows. His early education was obtained at Midhurst, in Sussex. He went thereafter to Oxford, and there obtained his A.M. degree in 1821. Whilst at Oxford he had the advantage of attending Dr Buckland’s lectures, then Professor of Geology. On leaving the university, he studied for the English bar; but finding this line of life not likely to be congenial, and having the means of living without the aid of a profession, he betook himself to geology. The seed sown by Dr Buckland had been dropped into soil fitted to its germination and rapid develop- ment. Probably Lyell’s first paper was an account of a “ Recent Formation of Freshwater Linn stone in Forfarshire,” his native county. This was very soon Allowed by many other papers, written at places visited by him in Hampshire and Dorsetshire. These were read before the Geological Society of London, of which he had become member. In the year 1824 he had shown such knowledge of geology, that he was elected one of the Honorary Secretaries of the Society. In 1827 he contributed to the “Quarterly” a review of Mr Poulett Scrope’s “ Geology of Central France.” Shortly afterwards, he published his “ Principles of Geology,” the work in which he first showed his distrust of old geological maxims, and started his own original conceptions. Most geologists before his day had attempted to explain many things by assuming that the natural agencies of bygone times had been much more powerful than now. On the other hand, Lyell maintained that the natural agencies now on our planet were capable of producing all the effects observed, if only sufficient time was allowed for their operation. These new views attracted great attention. The demand for the book in which they were explained was so great, that it went of Ed in b urgh , S^ss io i i 1875-76. 7 through five editions in a very short time— each edition contain- ing a large amount of new matter. The work, by these numerous additions, became so changed in character, that he reconstructed it, and brought out a new work called “Elements of Geology,” and greatly altered his “ Principles ” as regards arrangements. In the latter, he presented explanations of the various forces at work in the earth and in the universe likely to affect the earth. In the former, he described the observed effects. Subsequently he brought out the “Student’s Manual of Geology,” in which he brought together most of the facts mentioned in the two previous works. No geologist before LyelPs time had devoted himself so exclu- sively and so laboriously to the science. He not only kept himself acquainted with the discoveries made by others, but he travelled over large portions of the earth’s surface, with the view of verify- ing alleged facts, and making di coveries himself. He went to Norway, Sweden, Belgium, Switzerland, Germany, Spain, Catalonia, and the Danish islands of Seeland and Monen. He was twice in America. On the first occasion, in 1841, he went, in compliance with an invitation, to deliver a course of lectures at Boston. He then remained in the New World a whole year, his explorations extending from Canada through the States to the mouths of the Mississippi. On returning to England, he pub- lished his “ Travels in North America,” in which, whilst geological information chiefly is given, some useful views occur on other subjects also. In 1845 he paid a second visit to America, and examined more particularly the Southern States and the coasts bordering the Gulf of Mexico. On his return to England, he published his “Second Visit to the United States,” — a companion to his former work. The most recent of Lyell’s important works was his “ Antiquity of Man,” which went through four editions, the first having come out in 1863, the last in 1873. But beside these elaborate works, he published numerous memoirs, most of which had been read at meetings of the Geological Society and British Association for the Advancement of Science. In 1836, and also in 1850, he was President of the London Geological Society. The "Royal Society’s Copley Medal was awarded 8 Proceedings of the Royal Society to him in 1858, and the Geological Society’s Wollaston Medal was awarded to him in 1866. In the year 1864 he presided at the Bath Meeting of the British Association for the Advancement of Science. He was Patron of the Scotch Geological Society. In the year 1848 he was knighted, and in the year 1864 he received a baronetcy in recognition of his services to science. Sir Charles Lyell was married in 1832 to Mary Elizabeth, eldest daughter of the late Leonard Horner, himself a distinguished geologist. Lady Lyell was a devoted wife, and sympathised with her husband in his pursuits, accompanying him in all his travels, and assisting him in literary work. During the last five or six years, Sir Charles Lyell lost his eye- sight to such an extent that he could neither read nor recognise his friends. The last time that I was in his house, Harley Street, London, Lady Lyell had to lead him, and make known to him the presence of several friends who came in. Lady Lyell’s death in the year 1874 was a severe shock to her husband. After that event, Sir Charles’s health rapidly failed. His death was caused by a severe fall on the staircase of his house, he having, owing to his blindness, missed the uppermost step. Probably few men were ever so devoted to any special object, as Sir Charles Lyell was to geology, through his whole life. He was inspired by a genuine love of truth, and for its sake did not hesitate to retract opinions when he found he was mistaken. In the three first editions of his “ Antiquity of Man” he had expressed his concurrence in the opinion of some Scotch geologists, that the land near the Firth of Forth had risen 25 feet since the Homan occupation. In the last edition of the work, he revoked that concurrence. In the account given by him of the Glen Roy terraces, he published his belief, that they were due to fresh water lakes. In a letter which I received from him shortly before his death, adverting to some facts recently discovered, he allows, that perhaps after all, Darwin’s theory of the terrace having been made by the sea, might prove to be correct. Sir Charles Lyell in this respect showed an example to all men of science, in caring more for the interests of truth, than for mere consistency. 9 of Edinburgh, Session 1875-76. William Edmond Logan, another Honorary Fellow of the Society, was bora at Montreal, Canada, in the year 1798, and died on 22d June 1875. His father was originally a landed proprietor in Stirlingshire, and emigrated to Canada. He sent his son from Canada, when very young, to Scotland, to be educated in the High School, and after- wards in the University of Edinburgh. When young Logan was in Edinburgh, geological investigations and speculations were exciting much interest, in consequence of the discussion between the Huttonians and Wernerians. Mr Logan then acquired a taste for geology; and having occasion to go to South Wales, he began to study the rocks in the coal-fields there, at this time, beginning to be more extensively worked. Having procured an Ordnance Survey map on a large scale, he was at the trouble to trace out and lay down upon it the outcrop of all the coal seams worked through extensive tracts of country. Seeing where the outcrops ceased to be continuous, he ascertained the amount and direction of the dykes and slips by which the strata had been dislocated. He descended into the mines, and studied for himself the structure of the coal, and examined particularly the fossils found in the coal. He was then struck bv the fact, that every coal seam lay upon a bed of blue-coloured clay, in which apparently the plants had grown, now found petrified in coal. In several instances he discovered that some of the fossil trees which had their trunks in the coal-bed had their roots still stretching into the underlying bed of clay. About this time Sir Henry de la Beche, who was directing the Geological Survey of England and Wales, happened to come into South Wales. Having heard of Mr Logan, he became acquainted with him; and having seen the work he had been carrying on, he at once put him on the staff of the survey. Mr Logan having permanently adopted geology as a profession, became a Member of the Geological Society of London. Frequently joining in the discussions there, he made the acquaintance of Sir Charles Lyell, Sir Roderick Murchison, and other leading geologists. Having obtained leave of absence to visit his father in Canada, he went there in 1841, and spent much of his time in exploring the great coal-fields of Nova Scotia and Pennsylvania. VOL. IX. B 10 Proceedings of the Uoyal Society In the spring of 1842 he returned to England, and in the Gi-eological Society gave an interesting account of his survey in these American coal-fields. He had been particularly anxious to obtain a confirmation of his discovery, that coal seams everywhere rested on fire-clay; and he was able to afford these proofs from what he bad seen in Nova Scotia. He had made another discovery in these coal-fields. He had discovered the footprints of a reptile; and he brought to London with him the sandstone slab which contained these prints. This slab was submitted to Professor Owen, who expressed a clear opinion, that the impressions had been made by an animal which had four claws on the two fore feet, and three claws on the hind feet. The interest attaching to this discovery was, that no reptile had been discovered in rocks so old, it being at the bottom of the Carboniferous formation; — whereas, previously, no reptiles had been found below the Permian rocks. I mention this discovery of Logan’s, because I see that my friend Principal Dawson of Montreal, in his “ Book on Acadian Geology,” mentions that discoveries of similar reptiles, made in the year 1844 in Sweden and the United States, -had been asserted to be prior to others of the same kind. Logan’s reputation as a geologist was now established. It led to his being entrusted with the charge of the Canadian Geological Survey, on the recommendation of Sir Roderick Murchison and Sir Henry de la Beche. The Canadian Legislature had wisely resolved to have the mineral riches of the country ascertained by competent surveyers. F or nearly thirty years Sir W illiam conducted the Canadian Survey,, and drew most important conclusions regard- ing the whole series of rocks in that part of the world — conclu- sions universally accepted by geologists as correct. At the Paris International Exhibition of 1855, he showed a large collection of specimens, besides magnificent m^ps and diagrams, which attained much attention, and received great commendation. It was on this occasion, that the British Government, in recogni- tion of his eminence as a geologist, and of his services in Canada, bestowed on him the honour of knighthood. Sir William did not publish anything beyond the official reports of his survey. He was not ambitious of fame, either as an author of Edinburgh, Session 1875-76. 11 or otherwise. He stuck closely to the work he had undertaken, and continued at it till the year 1869, when failing health led him to resign. He, however, continued to take an interest in geological pursuits, and gave, from his private funds, a donation of L.5000, for the endowment of a chair of' geology in the M‘Gill College, Montreal. Charles Wheatstone was born at Gloucester in 1802, and died in Paris 19th October 1875. He was on the list of our British Honorary Fellows. The rudiments of education were obtained by him at a private school. Whether he afterwards went to a university, I have not discovered. His youth and early manhood were devoted to the construction of musical instruments, and to experiments with the view of dis- covering more exactly the laws of sound. He paid special attention to the instruments depending on vibrating springs. The present improved Concertina is due to his invention. His first scientific memoir was in the year 1823, when he pub- lished in the “ Philosophical Annals” an account of some “ New Experiments on Sound.” It excited considerable attention among physicists, and was translated into several foreign periodicals. In 1827, in the “ Quarterly Journal of Science,” he published farther “ Experiments on Audition,” accompanied by a description of the Kaleidophone, an instrument to illustrate both acoustical and optical phenomena. During the next eleven years, he continued to produce papers and to invent instruments for illustrating the properties of sound. In 1838 he seems to have entered on a different subject of inves- tigation altogether, viz., light. He had discovered relations be- tween waves of sound and waves of light. He communicated to the Royal Society of London, and also to the British Association^ an account of some hitherto unobserved phenomena of binocular vision, illustrating them by means of the instrument vhich he invented, called the “ Stereoscope.'1 To Wheatstone is due the discovery, that the conception of solidity is due entirely to the mental union of two dissimilar perspectives. In 1852 he invented an instrument called the u Pseudoscope ,” 12 Proceedings of the Royal Society which still farther illustrated the mental action in certain optical phenomena. An article in the “Edinburgh Review” of October 1858, describes thus the effect of the Pseudoscope: — “When an observer looks with it at the interior of a cup or basin, he not un- frequently sees it at first in the real form, but by prolonging his gaze, he will perceive the conversion within a few minutes ; and it is curious, that while this seems to take place quite suddenly with some individuals, as if the basin were flexible and were suddenly turned inside out, it occurs more gradually with others, the con- cavity slowly giving place to flatness, and the flatness gradually rising into convexity.”* Wheatstone was exceedingly interested in this discovery of the interference of mental action with optical phenomena, and invented several instruments with the view of ascertaining the principles on which it depended. The subject led him to study the subject of nervous organisation ; but it is believed, that he effected no special discoveries in that field. In 1834 the science of Electricity began to occupy Wheatstone’s attention. He endeavoured to ascertain the velocity of the elec- trical current. He invented many most ingenious machines with that view. He seems to have made only an approximation to the truth, viz., that the current travelled through a mile of wire in less than the 360th part of a minute. It now occurred to him that electricity might be employed in conveying intelligence along great distances by moving a magnet. By this time an idea of the same kind had occurred in G-ermany. Mr Cooke, when there, had become informed of the investigations by Schilling, and having come to London, made these known to Wheatstone. A proposal for a partnership between the two, was suggested, and was carried out. Messrs Cooke and Wheatstone A curious circumstance, analogous to the phenomena here described, was, without the help of any instrument, observed by me and other friends lately, in watching the revolutions of a cup anemometer on the top of Alnwick Castle. On looking at the instrument, it was seen revolving in a direction consisting with the truth ; but on continuing to look at it, in about half a minute the anemometer suddenly appeared to change the direction of its rotation, and to continue so to rotate. We remained for some time looking at the instrument to repeat the experiment. The same result on every occasion followed, and to every one of the party, eight or nine in number. 13 of Edinburgh, Session 1875-76. soon thereafter were employed to establish electric telegraphs on most of the great English railways. In 1837 the five-needle telegraph was invented; in 1840, the alphabet dial telegraph; in 1841, the type-printing telegraph; and the automatic telegraph between 1858 and 1867. By this last machine it was found possible to transmit words at the rate of from 100 to 160 words per minute. In 1840 Wheatstone conceived the idea of a submarine telegraph cable, and pointed out both the difficulties and the means of obviating them. His last work was to contrive a new recording instrument for submarine cables, formed by a globule of mercury moving to and fro in a capillary tube containing acid, or by a drop of acid in a tube containing mercury, and which was found to be 58 times more sensitive than any recorder previously employed. He had gone to Paris to exhibit this invention to his colleagues of the Academy of Science, when he was attacked by the fatal illness — bronchitis— which terminated in his death. This brief notice of Wheatstone’s discoveries in the science of sound, optics, and electricity gives but a poor idea of the immense amount of brain work which he went through in the long life accorded to him. The papers which he contributed to Societies both in Great Britain and on the Continent are very numerous. They were always characterised by great lucidity of style and by copious and telling illustrations, which made them both attractive and instructive. Wheatstone was elected a Fellow of the London Royal Society in 1836, a Chevalier of the Legion of Honour in 1855, a Foreign Member of the French Institute in 1873. In 1868 the Govern- ment of Lord Derby conferred on him a knighthood. In private life Sir Charles Wheatstone had 'the reputation of being reticent and unsociable. The fact probably was, that his mind was constantly absorbed with the problems which were con- stantly presented to it. He was so nervous and bashful, that though always ready and pleased to describe his discoveries to any single individual, he entirely broke down when he attempted to address an audience. Hence, his Professorship of Natural Philo- 14 Proceedings of the Royal Society sophy in King’s College, London, was little better than a title ; for he never had a class. There was no physicist of his time so universally respected. His remains were brought from Paris for interment in the family burial place at Kensal Green. The procession was followed by a vast number of carriages, including many of the nobility; and even the shops in the streets along which the funeral cortege passed were shut, whenever it was known whose it was. David Aitken, D.D., who had been seven years an Ordinary Fellow of this Society, was born about the beginning of this century. He died on the 27th March last, in his own house in Charlotte Square, Edinburgh. He was educated at the High School and University of Edinburgh, and became a licentiate of the Church of Scotland. I believe that he had been tutor in the family of the Earl of Minto, by whom, or through whose influence, he was in the year 1829, presented to the parish of Minto. There he remained minister for thirty-seven years ; and on resigning his charge, pur- chased a house in Edinburgh, where he- lived till his death. Being fond of travel, he visited Norway, Italy, Egypt, and Syria. As he suffered extremely during the winter season from delicacy of chest, he often spent the winter abroad. Possessing an independent fortune, he was able to obtain the services of an assistant during his absence. He was a person of literary tastes, was well acquainted with the German language, and was a friend and correspondent of the German philosopher Hegel. In the year 1827 he wrote an article in the “Edinburgh Review” on German literature. He also drew up the Statistical Accounts of Minto Parish, embodying an excellent account of its geology, botany, and zoology. His knowledge of Church history was so considerable that he was offered the Chair of Church History in the University of Edin- burgh. On his declining it, the late Dr Welsh was appointed. His sermons were in composition marked by great elegance and clearness ; but owing to delicacy of chest, his voice was weak, and his manner in the pulpit had not the earnestness necessary to create interest. He was exceedingly fond of natural history, and took great of Edinburgh, Session 1875-76. 15 interest in his garden, which was always kept with scrupulous neatness. John Hughes Bennett was born in London 31st August 1812, and died at Norwich 25th Sept. 1875. He had joined our Society in 1842. He was educated at the Grammar School, Exeter. It is stated, however, that he was indebted for the early part of his education to his mother, a lady of brilliant intellectual attainments. Being a great admirer of Shakespeare, she caused her son to read aloud to her many of his plays, and as he did so, taught him the art of emphasis and rhetorical action. Probably to this tuition of his mother, Dr Bennett was indebted for the elegance of his composi- tion, and for the impressiveness of his delivery when he lectured or spoke in public. He commenced the study of medicine at Maidstone, in the year 1829, under the guidance of a practitioner there. It was there that he acquired the art of dispensing, and even obtained a certain amount of medical practice. He assisted also in post-mortem examinations. To acquire better medical instruction and training, he removed to Edinburgh in the year 1833, — unacquainted with any one in that city or in Scotland. By his talents and assiduity he soon attracted the notice of his professors, and obtained the esteem of numerous fellow-students. His attention was devoted chiefly to anatomy, physiology, and pathology. Having joined the Royal Medical Society, and shown his abilities and knowledge at its meetings, he ultimately became President of the Society. Whilst still a student, in the year 1836, he published two papers which obtained for him considerable credit. In the year 1837, he received the degree of M.D. with the highest honours, obtaining at the same time a gold medal for his thesis. After obtaining all the knowledge which Edinburgh could supply, Dr Bennett repaired to Paris, where he studied for two years. Being able to speak and write the French language fluently, he wrote in the French medical journals, and ultimately became President of the Parisian Medical Society. 16 Proceedings of the Royal Society He also went to Germany, spending some time in the principal University cities, and endeavouring to acquire knowledge beyond what he had already obtained. One of his acquisitions on the Continent was ability to use the microscope in practical medicine. Nor was his pen idle, for whilst abroad, he contributed no less than seventeen articles to Tweedie’s “ Library of Medicine.” In 1841 he returned to Edinburgh, and commenced a course of lectures on histology. He there took the opportunity of showing to what an extent the microscope might and should be used. It was at this time that Dr Bennett published a treatise on the use of cod-liver oil as a therapeutic agent in certain forms of gout, rheu- matism, and scrofula, — dedicating the treatise to Sir Robert Christison. In Germany he had seen the good effects of using this medicine in these cases. From 1842 to 1848 he continued to give lectures on various medical subjects. In the last named year he was appointed to the Chair of Institutes of Medicine, vacant by the transference of Dr Allen Thomson to Glasgow. For several years Dr Bennett was proprietor and editor of the “ Edinburgh Monthly Journal of Medical Science,” in which, besides editorial articles and reviews, he inserted multitudes of separate memoirs. In the “British Medical Journal,” where a detailed account of Bennett’s life and labours is given, and from which I have culled the foregoing notices, I see a list of no less than 105 memoirs on various anatomical and pathological subjects. In July 1848 Dr Bennett was unanimously elected to the Chair of Institutes of Medicine. Whilst teaching in the University and in the Infirmary, Pro- fessor Bennett found time for literary work, and published his highly appreciated “ Clinical Lectures on the Principles and Practice of Medicine.” This book passed through five editions in this country, and six in the United States, besides being translated into French, Russian, and Hindoo. The following additional works flowed from his ready pen. Their titles were, “Pulmonary Consumption,” “Cancerous and Cancroid Growths,” Introduction to Clinical Medicine,” “Outlines of Edinburgh, Session 1875-76. 17 of Physiology/’ “ Text-Book of Physiology — General, Special, and Practical.” Professor Bennett had conferred upon him numerous honours and distinctions. He was President for two years of the Medico-Chirur- gical Society of Edinburgh ; Hon. Secretary and emeritus President of the Royal Medical Society of Edinburgh ; and Fellow of numerous medical societies on the Continent. He bad sent to him, about a year before bis death, a special licence from the French Govern- ment entitling him to practise medicine in France. This honour was probably suggested by the fact of his having, two or three years before his death, resided in the south of France for the benefit of his health. The enormous amount of work, both mental and physical, which Professor Bennett undertook, probably shortened his life. About 1865 his first illness appeared in the form of a throat affection. Having recovered by a sojourn in the south of France, and returned to Edinburgh, he was again prostrated in 1869. After an interval he recovered, but in the winter of 1871-2 he was obliged to return to Mentone. During the following summer, he resumed work in Edinburgh, and gave some clinical lectures. The winters of 1872-3 and of 1873-4 again forced him into a warmer climate, but each time with less benefit. In the year 1874, he resigned the Chair of the Institutes of Medicine. Last winter he spent in Nice. His last illness was owing to disease of the bladder. In August last he returned to Norwich, the place of his birth, where an operation was performed, and a stone was extracted. The debility caused by this operation, combined with previous exhaustion of constitution, brought on death. Undoubtedly, Professor Bennett was in the medical profession a person of great eminence. He introduced many very important changes in medical practice, and made known many new principles. His devotion to study and investigation probably led to his having the character of being somewhat unsociable and austere. But those who had the privilege of intimacy with him, know that he was truthful, honest, honourable, and earnest in every relation of life. The Rev. Dr Thomas Jackson Crawford joined our Society in vol. IX. c 18 Proceedings of the Royal Society 1871. He was born in 1812, and died lltli October 1875, at G-enoa, at which place, when he died, he was sojourning for the benefit of his health. His father was Professor of Moral Philosophy in the United College of St Andrews. His son Thomas received the earlier part of his education at the Edinburgh High School. To St Andrews he went back for his more advanced studies. Intending to be a clergyman of the Scotch Church, he took his degree in 1831, and in 1834 was licensed as a preacher of the gospel by the Presbytery of St Andrews. Whilst at college he attracted the special notice of the professors by the superiority of his talents, his assiduity to learn, and the excellence of the essays which he produced. The patronage of the parish of Cults being in the gift of the Principal and Masters of the United College, he was presented to that parish. When the Royal Commission on Church Patronage in Scotland sat, it inquired into the way in which the University of St Andrews exercised its ecclesiastical rights. On that occasion the Rev. Dr George Cook, one of the Professors of St Andrews, explained to the Commissioners the circumstances attending Mr Crawford’s presentation ; adding, that though his own son was then desirous of obtaining it, and though there was a party in Cults parish wishing his appointment, he did not hesitate to prefer young Crawford to his own son. Whilst minister of Cults, he wrote a Statistical Account of the parish, which, besides other information, contains several interest- ing anecdotes regarding the youthful career of Sir David Wilkie, the painter, whose father had been minister at Cults. From Cults, Mr Crawford was translated to Glamis, and six years later he was promoted to Edinburgh, to be minister of St Andrew’s Church, jointly with the late Rev. Dr Thomas Clark. About this time he received from his alma mater University, the degree of D.D. He also, shortly thereafter, was made Convener of the General Assembly’s Committee on Psalmody, an appointment for which he was well fitted, on account of his knowledge of and fondness for music. Having preached a sermon in 1847 on Jewish Missions, which was afterwards published, that circumstance led to his being selected of Edinburgh, Session 1875-76. 19 to take the oversight of the G-eneral Assembly’s Scheme for the Conversion of the Jews. In 1853 he entered the arena of controversy by publishing first a pamphlet, entitled “ Presbyterianism Defended against the Exclu- sive Claims of Prelacy,” and thereafter another pamphlet, entitled “Presbyterianism or Prelacy; which is the more conformable to the pattern of the Apostolic Churches.” His views on these sub- jects were reiterated by Dr Crawford in the Address which he delivered from the Chair of the G-eneral Assembly, as Moderator, in the year 1867. This public advocacy of Presbyterianism, to the prejudice of Prelacy, drew forth some letters from Bishop Words- worth, which were published in the “ Scotsman ” newspaper, “The Fatherhood of God” was Dr Crawford’s first important contribution to purely doctrinal subjects. Dr Candlish, some of whose views were controverted, replied to this publication. At this time Dr Crawford was Professor of Divinity in Edinburgh University, having succeeded the Rev. Principal Lee in the year 1859. He published also a volume on the “ Atonement,” in the year 1871. In the year 1874 he was appointed the Baird Lecturer. His lectures, first delivered in Glasgow, were afterwards, by special request, re-delivered in Edinburgh, and were published in a volume under the title of “ Mysteries of Christianity.” The immense amount of study which these lectures entailed, I have heard, weakened Dr Crawford’s health, and prepared his con- stitution for the illness to which he ultimately succumbed. In the winter following the publication of these lectures, he was obliged to reside in the milder climate of the south of England. He suffered from great delicacy of lungs. But he returned to Edinburgh last spring, whilst the sharp east winds were still pre- vailing, and moreover betook himself again to College work, against the advice of his medical friends. During the summer of 1875 he went to Germany, sojourned a while in Switzerland, and then went to Italy. There he so far recovered his strength, that he could walk considerable distances, and even up steep hills, without suffering inconvenience. But the weather in the north of Italy is often dangerous to persons with 20 Proceedings of the Royal Society weak lungs, especially when the wind is from the north. After a short illness of ten days, caused by inflammation of the lungs, lie died. Dr Crawford, besides being a man of great eminence, and most highly respected in his own profession, was a person of varied attainments. Besides having a knowledge of music, he often took his part at amateur vocal concerts, with others — some of whom are probably now present among us to-night — and who, I am sure will bear me out when I say, and I say it from a long personal acquaintance with him, that Dr Crawford was a person of most amiable disposition, and most conciliatory in all the relations of life. Though he entered into controversy he ever avoided personal aspersions ; and those with whom he fought, were always ready to admit the fairness with which he wielded his weapons. I learn from Dr Crawford’s son, what I had not been aware of, that Dr Crawford kept up to the last, his knowledge of mathematics; and that frequently, when he was in want of recreation, nothing pleased him more than taking a problem and working it out. Sir William Jardine, Bart, of Applegarth, in the county of Dumfries was born in February 1800, and died 21st November 1874, He had been fifty years a member of this Society. He was the son of the sixth baronet, by a daughter of Thomas Maule, the representative of the Earls of Panmure. Born in Edinburgh, he was educated partly at home, partly at York. With a view to the medical profession, he attended the medical classes in Edinburgh. But he did not carry out these professional views. Having succeeded his father when he was scarcely twenty-one years of age, he took up his residence at his family dwelling-place, Jardine Hall. By this time he had evinced a strong taste for scientific pursuits, especially natural history in all its branches. He was a good botanist, a good geologist, and a good ornitho- logist. He was also a keen sportsman, both with the gun and the rod. Very many specimens in the large and valuable museum which he formed at Jardine Hall, were collected by himself. In the year 1825 he commenced, in conjunction with the late Mr Selby of Twizell, in Northumberland, the publication of the 21 of Edinburgh, Session 1875-76. “ Illustrations of Ornithology.” In 1833 he undertook a still more important work, “ The Naturalists’ Library,” forty volumes of which appeared in the course of the next ten years — a work for which he obtained contributions from the best scientific naturalists in the kingdom; — but of this work, no less than fourteen volumes are made up of contributions by Sir William exclusively. He also published a new edition of Alexander Wilson’s “ American Orni- thology;” started and carried on for some time a magazine of zoology and botany ; and was also for some years a joint editor of the “Edinburgh Philosophical Journal.” Here is a list of other works which flowed from his pen New edition of “White’s Selborne,” “British Salmonidse,” “ Ichthyo- logy of Annandale.” A still more important work by Sir William Jardine was en- titled “Contributions to Ornithology,” in three volumes, extend- ing from the year 1848 to 1852. This work contains descriptions and coloured figures of many species of birds previously unknown. Another publication was “ Memoirs of the late Hugh Edwin Strick- land,” in the year 1858. Mr Strickland had married a daughter of Sir William. He was a good geologist. He unfortunately was killed in a railway tunnel, the rocks of which he was examining when a train came on him unexpectedly. Jardine’ s frequent visits to Northumberland, to co-operate with his friend Mr Selby of Twizell, brought him into acquaintance witli Dr Johnston of Berwick-on-Tweed, who was well versed in botany and marine zoology. Dr Johnston having about this time founded the Berwickshire Naturalists’ Club, Sir William Jardine joined it in September 1832, and in that year contributed papers of some value on the “Parr” and the “Silver White,” small fish of the salmon species, which frequented the Tweed and many other rivers. At that time, the true nature of these fish was not known, though it has since been well ascertained that the parr are the young of the true salmon in their first year’s growth. Sir William Jardine was President of the Berwickshire Natura- lists’ Club in the year 1836, and frequently attended its meetings in subsequent years. In the year 1860 he was one of the’ Royal Commissioners appointed to investigate the Salmon Fisheries of England and 22 Proceedings of the Royal Society Wales. The evidence collected by these Commissioners is of great value. Legislation followed on their report. Shortly before his death, Sir William occupied himself in pre- paring a catalogue of the various objects of interest in his museum. This catalogue was in proof, and awaiting revisal when he died. The list of birds contains no less than 6000 species, and probably not less than 12,000 specimens. Sir William was most obliging in lending specimens to friends. I remember on one occasion obtaining from him on loan the skull of a fossil bear found in this country, on the occasion of a popular lecture which I was giving in Berwickshire. Sir William Jardine was during the last ten years of his life constantly resident at Jardine Hall, enjoying the sports of country life, discharging the duties of a proprietor, and taking his share of county and parochial business. William Macdonald was born in the year 1798, and died on 1st January 1875. He was the oldest member of our Society, in the class of Ordinary Fellows, having joined the Society in the year 1820. There is, however, one older member, my venerable friend Sir Richard Griffiths, who is an Extraordinary Fellow of the Society. He was ninety-one years of age last September, and is still in excellent health, residing near Kelso. I believe that Sir Richard would have been here to-night, had the weather been less stormy. Dr Macdonald at an early age inherited a good estate in Argyll- shire. He applied himself to the execution of extensive works in that county, for the improvement of his property, and of the district where it was situated. Unfortunately he involved him- self in financial difficulties, and was obliged to sell his estate. He then studied medicine, passed with honours, but never practised. In 1820 he joined a number of Societies. He was the oldest member not only of our Society, but also of the Royal College of Physicians and of the Linnean Society. Dr Macdonald frequently read papers to us on various subjects. He held peculiar views on some points of anatomy, which were 23 o f Edin burgh , Session 1875-76. entirely at variance with those generally held ; but he never would concede that he was in error. He was very partial to natural history, and wrote upon “ The Structure of Fishes,” “ The Unity of Organisation, as exhibited in the Skeleton of Animals,” and “On the Vertebral Homologies, as applicable to Zoology.” In the year 1849 he accepted an appointment to that somewhat anomalous professorship of “Civil and Natural History” in St Andrews, but I am not sure whether he ever had any students. He had formed a large and interesting collection of specimens in natural history and anatomy. Principal Shairp informs me that, a few years before his death, Dr Macdonald made over this collection to the University Museum. Donald Mackenzie became a Fellow of this Society in 1870. He was born 19th June 1818, and died 17th May 1875, at Nor- wood, near London, where he had gone on account of ill health. Though born in Edinburgh, his father was from Sutherlandshire, and a Captain in the Royal North British Fusiliers. His mother was Robina Jamieson, one of the seventeen children of John Jamieson, D.D., who wrote the well-known Dictionary of the Scottish language. Donald was the eldest of seven children, all of whom he survived, though he, too, died at the comparatively early age of fifty-seven. At first he studied for medicine, and received the degree of M.D. from the University of Edinburgh in 1838. He was also a Fellow of the Royal College of Surgeons. But he abandoned that profession, and came to the Scottish bar, influenced, it is believed, by the expectation that as his uncle, Robert Jamieson, advocate, had a large amount of practice in the Courts, he would be able to give him a lift. Robert Jamieson I remember well in the Parliament House, being the most con- spicuous figure there for height and breadth, and a lawyer of great acuteness. His sister, Donald’s mother, lived to the age of eighty- four. Donald, to whom this notice refers, did not inherit the Jamieson constitution. He was narrow-chested and slim, but walked with elastic step. 24 Proceedings of the Royal Society Having come to the bar in 1842, he soon got into considerable practice, and was popular among his brethren in the Parliament House. He was appointed Advocate-Depute in 1854, an office which he held till 1858, when he lost it on a change of Grovern- ment. He was reinstated in 1858, and was appointed Sheriff of Fife in 1861. In the discharge of this office, he is said to have given great satisfaction, both to the practitioners in the Sheriff- Court and to the resident gentry. Mr Mackenzie was raised to the Bench in 1870, and was not only most conscientious in his attention to the judicial duties, but was successful in pronouncing judgments which were seldom reversed. It is related that on two occasions, when they were reversed in the Inner House, they were, by an appeal to the House of Lords, adhered to. Lord Mackenzie was exceedingly fond of all country sports. A serious illness was contracted, about two years before his death, in consequence of his continuing to fish in wet clothes, till he got a severe chill. In November 1874 he became so ill, that he was obliged to ask leave of absence for the winter. During the subse- quent Christmas holidays, he attempted to return to his work in the Bill Chamber, but he was obliged to give it up, and confine himself to bed. Disease of the heart, aggravated by rheumatism, had set in. He continued more or less an invalid for a whole year before his death, seldom discharging any judicial work. Lord Mackenzie was universally respected for his close attention to duty, his sound knowledge and judgment as a lawyer, his freedom from guile, and his conciliatory disposition toward all with whom he was brought in contact. His life was shortened by a determination to perform any duty incumbent on him, though probably conscious that he was thereby weakening his constitu- tion. John Sinclair was born 20th August 1797, and died 22d May 1875. He was the third son of the Right Hon. Sir John Sinclair, Bart, of Ulbster, in the county of Caithness, author of that valuable repertory, the Statistical Account of Scotland. His mother was Diana, daughter of Alexander, the first Lord Mac- donald. 25 of Edinburgh, Session 1875-76. His education commenced in Edinburgh University; but he went afterwards to Pembroke College, Oxford. In the last book which he published, entitled “ Old Times and Distant Places,” he mentions that, when at Edinburgh University, he was the chief means of forming what was called the “ Rhetorical Society,” among the members of which were the present Earl of Wemyss, the late Adam Anderson (afterwards Lord Anderson), and David Robertson, who, whilst on his death-bed, was created Lord Marjoribanks. When he went to Oxford, he proposed a similar society; but “the Dons” (he says) “ frowned upon him, and prevented it.” The project was renewed some years after. The “ Oxford Union Club” was then formed, embracing among its members the present Archbishop of Canterbury, Mr Gladstone, Mr Lowe, and others who afterwards became men of distinction. Having gone through the necessary forms for taking orders in the Episcopal Church, he was ordained by the Bishop of Lincoln in 1820. He was shortly thereafter appointed to St Paul’s Episco- pal Chapel, Carrubbers Close, where he remained till he became assistant to the Rev. Mr Alison, the officiating clergyman of the then new and handsome chapel of St Paul’s, in York Place. It was in the year 1820 that Mr Sinclair joined our Society. I see from his little book, that he took a considerable interest in our proceedings, as he mentions our Dinner Club, of which he was a member, and specifies several duties which he undertook as a member of Council. Thus he was selected by the Council to endeavour to induce Dr Williams, rector of the English Academy, to shorten the length of a paper he was to read on Greek particles, a subject on which he had read several long papers before, much to the ennui of the majority of members. Dr Williams, it seems, was not a person who could be easily diverted from bis purpose ; Mr Sinclair under- took to try his hand upon the inflexible Welshman. He explains, in an amusing way, how he succeeded. Another more important work with which Mr Sinclair was entrusted by our Council, was the arrangement of the unpublished MSS. of Hume, the historian. These MSS. had been left as a legacy to the Society by the late Baron Hume, the historian’s VOL. XI. D 26 Proceedings of the Royal Society nephew. In this duty he was conjoined with the late Lord Meadowbank and Dr Abercrombie; but the chief part of the work fell on Mr Sinclair. He mentions that it was in the year 1828 that he became acquainted with Dr Thomas Chalmers, when the latter resigned his professorship of Moral Philosophy at St Andrews, to become Professor of Divinity in E linburgh University. Having a great admiration for the doctor’s character and writings, he attended his first course of lectures, and describes the intense interest with which he and the other students listened to the professor’s exposi- tions. The salary of the professors being then very small — only £200 — the idea of offering a testimonial to Dr Chalmers, at the end of his first course, occurred to Mr Sinclair. According^ a sum of £200 was raised from the voluntary students, and presented to the new professor. In the year 1839 Mr Sinclair went to London, apparently to consult Mr Wardrop, the celebrated occulist, about his eyes. He had to submit to a painful operation and to severe discipline, which confined him to a room in London for some weeks. Whilst he was there, a vacancy occurred in the office of Secre- tary to the National Society — a great Society, established, among other things, for the encouragement and support of schools con- nected with the Church of England. Mr Sinclair was asked to fill the vacant office. At first he refused, as it would oblige him to leave Edinburgh altogether, and he could not be certain of being so well received in London as he had been in his own country. But finding that the two London Archbishops and other persons of influence were anxious that he should accept, he consented. He was at the same time appointed to be examining chaplain to the Bishop of London. Immediately after entering on this new office, he found himself involved in a great public controversy, which called for the utmost exertion, with great tact on his part. The controversy had reference to the schools of the National Society receiving aid from Gfovern- ment. After the administration of the Education Grant was transferred from the Lords of the Treasury to the Privy Council Committee, a system of inspection, to see that the schools were properly conducted as regards teaching, was resolved on. The of Edinburgh, Session 1875-76. 27 Church of England did not object to inspectors; but inasmuch as the religious instruction in the schools was to be reported on by Government inspectors, the Church desired to have some security as to the qualifications of the inspectors to judge of that in- struction. The National Society, at the suggestion of Mr Sinclair, resolved to intimate to Government that they would recommend the managers of all Church of England schools to refuse the Govern- ment grants, unless some arrangement satisfactory to the Church was made on that point. The Government having at first refused to make any concession, notice was sent to the Privy Council from the managers of about 200 schools, that they would not in future receive the grant. Mr Sinclair, in support of the National Society’s views, appealed to the Universities of Oxford and Cambridge, and secured their help. He preached on the subject ; he induced several of the leading London newspapers to advocate the views of the Church; he obtained the assistance of Lord Ashley and other influential public men. At length the Privy Council Committee yielded, — agreeing that no inspector should be allowed to examine any Church of England School whose name had not first been sub- mitted to the Archbishops of Canterbury and York for their sanction. This privilege was extended also to the schools in Scot- land connected with the Church. The grants to the Church of England Schools were paid to the Treasurer of the National Society, and were by him distributed to the schools. When the above arrangement had been completed, the office of treasurer was held by a Mr Watson, who was so averse to the proceedings of the Privy Council, that to avoid touching the unclean thing, he refused to receive the Government grant, or grant a receipt for it, and sent in his resignation. Mr Sinclair on this occasion was appointed to be treasurer, so that he was installed into the two most important and laborious offices of the Society. In the year 1843 Mr Sinclair, in addition to these duties, was called on to undertake important pastoral work. In that year he was appointed Vicar of Xensington, and in the following year Archdeacon of Middlesex. The population of that new part of London had immensely out- grown the means of public worship, so he set himself to work on 28 Proceedings of the Royal Society behalf of Church Extension. He remained Vicar and Archdeacon for the last thirty years of his life. When he came into the dis- trict there were three parishes ; before the close of his career, he had been the means of forming in it twenty-three parishes. Whenever Mr Sinclair found it necessary to carry any important measure in later years, he seems to have acted on a hint given to him by the late Dr Chalmers, on the last occasion, as he says, that he saw this great and good man. This was in the year 1843. He had been telling the Doctor of wrhat he was doing for the support and extension of the Church of England National Schools, and in particular, how' he had received promises of support from hundreds of influential people, including members of the Cabinet and of both Houses of Parliament. Dr Chalmers, he says, “heard me patiently for some time, and then replied, ‘ Mr Sinclair, I per- ceive you are an enthusiast; your National Society must, under G-od, depend upon the nation for support, and not on Cabinets or Parliaments.’ ” After this conversation, very little is said by Mr Sinclair in his autobiography about applications by him to influential individuals; whilst a good deal is said about the public meetings which he resorted to when he wanted to raise money, or to influence public opinion. He never spoke from the platform himself; for after leav- ing the University, he lost the fluency of speech, which he says, he had acquired there ; but he had great tact in arranging meetings and providing speakers who were likely to be listened to. Several amusing stories of this kind are told in his little book. One may be mentioned. Mr Thackeray had recently come to reside in Kensington, and Mr Sinclair thought his name would be a powerful attraction. Mr Sinclair called upon him. Thackeray was unwell, and in his bedroom. Mr Sinclair having sent up his card, Thackeray came down stairs, when Mr Sinclair explained his object. Thackeray at once declined, saying he had never in his life made a speech in public, and that he only wrote for the public; and besides he was too ill to leave the house. Mr Sinclair said that he would not insist on a speech, but that it wras very difficult to get up a meeting in Kensington, and that if Mr Thackeray would only allow his najne to be printed in the handbills, he would not insist on his saying much, and would have the speaking done by 29 of Edinburgh, Session 1875-76. others. Mr Thackeray was amused, and said, (c Well, if I am alive, I will come to your meeting.” The handbills were accordingly issued with Thackeray’s name in them. A great crowd assembled. Mr Thackeray appeared on the platform. He found when there he could not avoid saying something. His words were few but telling, and they were received with enthusiasm. Mr Sinclair adds, that this was the only time that the rhetorical powers of the great novelist were proved at a public meeting. It was not merely in London that Mr Sinclair was of use. During general periods of great distress in the manufacturing and mining districts of Wales and Lancashire, the bishops of these dioceses obtained his services to enable them to raise funds and devise measures of relief ; his services in these respects being thought of, on account of his well-known business habits, and also his sympathy with the working classes. In the year 1853 he was sent out to the United States as one of a deputation from the Church of England to the General Conven- tion of the Protestant Episcopal Church in New York. When there, he made acquaintance with Mr Washington, the nephew of the great man who had founded the American Republic, and with whom his father, Sir John Sinclair, had corresponded. I have had sent to me a long list of pamphlets, books, and sermons, published by the Archdeacon. The largest work is one in two volumes, published in 1837, on the Life and Times of his father. From what I have said, it will be perceived that Mr Sinclair, by the energy with which he threw himself into every work he under- took, justified Dr Chalmers’ opinion, that he was an enthusiast. But his enthusiasm was — which is rarely the case — tempered with great good sense and sound judgment. His untiring industry, his practical usefulness, and his benevolence of character, showed that he was no unworthy son of a most excellent and patriotic Scotchman. Having concluded all that it has occurred to me to state regarding ourselves — I mean regarding the work we are doing, and our means of doing it — I proceed to submit to you a few remarks regarding the present state of science generally in our own country. It appears to me that a great educational movement, amounting 30 Proceedings of the Royal Society almost to a revolution, is at present taking place in our land, and especially in that branch of public education which relates to science. I will not say that old institutions are being subverted; but undoubtedly new institutions are rising up very different from the old, and the old are undergoing considerable changes. I believe that the seed from which all these changes have sprung, and are springing, was planted by one man — the late Prince Consort. I know of no other person of weight and influence who so constantly took every opportunity of urging on the people of this country the introduction into our universities and schools of scientific instruction. This opinion is shared by others more entitled than me to speak on this subject ; to whom I will now shortly refer. Three weeks ago, at Oxford, His Royal Highness Prince Leopold agreed to perform the duty of distributing prizes to students of the School of Science and Art established in that town. The prince was introduced on that occasion by the Duke of Marlborough, lord- lieutenant of the county, and who, some years ago, was President of the Government Department on Education. His G-race, on in- troducing the prince, said that “it was not surprising that His Royal Highness should take a warm interest in every thing that belonged to Science and Art, when they remembered that he trod in the steps of the illustrious prince to whom the development of Science and Art in this country was mainly if not wholly attributable.” Prince Leopold responded to this sentiment. “ I do not forget,” said His Royal Highness, “ that there is devolved upon me, as well as upon other members of my family, a sacred trust, to foster, in such manner as we are able, the general study throughout the kingdom of Science and Art. From the passage I am about to read,” be continued to say, “ you will perceive that only a few years ago, and even in our university, Science and Art studies received little, if any, support. I will quote from an address by my revered father on the occasion of his laying the first stone of the Birmingham and Midland Institute, almost exactly twenty-four years ago.” The passage quoted by Prince Leopold, was a remarkable one. Its first sentence was as follows : — “ The study of the laws by which the Almighty governs the universe is our bounden duty.” Prince 31 of Edinburgh, Session 1875-76. Albert, in the passage so read by his son on this occasion, went on to show that, besides being our duty as human beings, it was for our interest as citizens to attend on these studies. “I advise you,” said the prince, “ to follow, in undivided attention, the sciences of mechanics, physics, and chemistry, and the fine arts of painting, sculpture, and architecture. You will thus confer upon your country an inestimable boon, and in a short time have the satis- faction of witnessing the beneficial results upon our national powers of production. Other parts of the country will emulate your ex- ample, and I live in hope that all these institutions will some day find a central point of union, and thus complete the national organisation.” Weighty as these words of Prince Albert were, and coming from an authority so much respected, I am not sure that they would have been universally listened to, had it not been for the great international exhibition of works of industry held in London in the year 1851 — itself a measure due to the sagacity of that excellent prince. There the people of this country first saw, with their own eyes, what were the fruits of the superior schools for scientific in- struction existing in Germany, Austria, Switzerland, and France. Shortly afterwards, royal commissions were issued to ascertain to what extent any of the sciences specified by the Prince Consort were taught in our schools. The result of these inquiries was sufficiently remarkable. In the year 1864 the Public Schools’ Commission, after special inquiry, reported that from all the first class schools in England, the teaching of science was practically excluded. This official exposure had some effect ; for in the year 1868 another Government commission, the Endowed Schools’ Commis- sion, reported, that a majority of the endowed schools in England had intimated their willingness and their intention to introduce science teaching. To how very small an extent this promise was fulfilled, may be judged of by the revelations of the Oxford and Cambridge school examinations made throughout England during the last three or four years. Even in this very year of 1875 what has been ascer- tained? Out of 461 candidates for certificates of good scholarship from 40 first-class English schools, there were only 28 scholars in 32 Proceedings of the Royal Society chemistry, 21 scholars in mechanics, 15 in physical geography, and 6 in botany; whilst for Greek there were 433 scholars, for Latin 438, and for elementary mathematics 458. The small amount of scientific instruction given in the English endowed schools was ascertained, still more precisely, by the Royal Commission, which has only recently framed its report. I mean the commission over which the Duke of Devonshire presided. From that report it appears that a circular was sent out by this commission two years ago to about 250 endowed schools, requesting them to fill up a sohedule showing what amount of scientific instruction, if any, was given in them. Only 128 answers were received'. That fact alone was significant. But when these answers came to be examined, it was found that out of the 128 answers, only 87 gave any definite information. Of these 87, 65 confessed to giving no science teaching whatever ; of the remaining 22, the utmost time allotted to any kind of scientific instruction, was four hours per week, in eighteen of the schools. But though it was right to ascertain the truth in this matter through the authentic inquiries of royal commissions, the people of this country, knowing well enough, from their own experience and observation how the matter stood, would not wait for these official inquiries. They took the matter into their own hands, and set to work at once to supply what was required. I do not know any stronger proofs of public patriotism in our country, than what this educational movement affords. In all the great centres of industry, arrangements were made for having institutions established in which not only science in its various branches should be taught, but the arts and literature also. At Manchester, John Owens bequeathed about L. 100, 000 for the endowment of a new college. No part of that money, however, being allowed to be expended on buildings, his fellow-citizens supplied what was needed. A sum of L. 250,000 was raised; and in the year 1870 the foundation stone of a magnificent edifice was laid for a Science and Art College, the Duke of Devonshire presiding. In the year 1871, a physical science college was established in Newcastle, for which L. 35, 000 was raised; and as it was to be affiliated with Durham University, that university agreed to give L.1000 a year out of its revenue for the institution. 33 of Edinburgh, Session 1875-76. In the year 1873, Josiah Mason, who had made a large fortune as a manufacturer at Birmingham and Kidderminster, gave the princely sum of L.250,000 (or the erection and endowment of a College of Practical Science in Birmingham. In January 1874, an association was formed for the promotion of scientific industry in Lancaster, at which the Earl of Derby pre- sided— an association formed chiefly at the instance of Lancaster manufacturers and artizans, who, having visited the Vienna Inter- national Exhibition held in the autumn of 1873, had seen there the rapid and alarming progress of Continental nations in many of the arts. In the same year, the Yorkshire College of Science was begun in Leeds, of which college Lord Frederick Cavendish is president, there being L. 100,000 subscribed for it. In the course of last summer, steps were taken to establish in Bristol a College of Science, to be affiliated to Oxford University, for which L. 26,000 has been already subscribed. Nottingham, Sheffield, and other towns, not so wealthy as to found colleges, are, however, stirring for the establishment of schools and societies for the teaching of classes. In Scotland, Dundee is stirring, wishing to have a college which is to be affiliated with St Andrews University, and for which it is proposed to raise as much as L. 200,000. Nor are our old, time-honoured national universities, in the midst of this great educational movement, asleep. Asleep or in- different they could scarcely remain, for very obvious reasons. Both at Cambridge and at Oxford, science lectures and fellowships have been at length introduced ; and the Chancellor of Cambridge, the noble Duke of Devonshire, has, from his own funds, presented that university with a splendid chemical and physical laboratory, having a most complete apparatus, at a cost of L. 10, 000. Our own University of Edinburgh has during the last five years had three new chairs created and endowed for engineering, geology, and political economy; and farther measures of extension, on a large scale, are being adopted, for which above L. 85, 000 have been already subscribed. Even the farmers , who are not generally proverbial for moving out of old paths, or even for moving in them, except at a slow pace, VOL. IX. E 34 Proceedings of the Royal Society are showing signs of progress. The Royal English Agricultural Society last year set apart L.500 to be given yearly in scholarships to encourage instruction in the sciences bearing on agriculture. The Highland and Agricultural Society has this year set apart L.250 for a similar purpose. But I must here offer a word of apology for the managers of the English endowed schools, which, in their programmes of studies, made no provision whatever for science. I remember when my son was at one of these schools, that I went to the head master and ventured to hint the disappointment I felt at the want of such pro- vision. His answer was— “ We are obliged to suit our teaching to university requirements. Only certain subjects are taught at Oxford and Cambridge ; and we endeavour to prepare our scholars in the subjects taught in these universities.” I thought the excuse satisfactory ; but now that the old univer- sities have introduced science teaching, and now that new colleges are being established all over the land with the same view, and bursaries are given by societies, corporations, and associations, in almost every large town, these secondary endowed schools will have no longer an excuse for not giving science instruction ; they will be even under a necessity to give it for their own sakes. Here again, however, I have to observe that the country refused to wait this slow progress of school amelioration. The G-overnment, with the entire approval of Parliament, by means of a special department at Kensington, encouraged the establishment through- out England and Scotland of schools and classes for the teaching of science and art. This encouragement was and is now given by prizes to scholars, remuneration to teachers, and loans of apparatus to the schools. The result has been marvellous. The scheme has been in operation for only nine years. At first it was little known and not well understood; but now these schools are extending rapidly; for whilst in the year 1869, that is three years after the scheme was started, there were in G-reat Britain only 523 schools with 24,865 scholars, there were in 1874 (since which date I have seen no reports), 1336 schools and 53,050 scholars. It is also proper to mention that the national elementary schools which are recognised by the Education Act for England and for Scotland, are encouraged to include various sciences in their pro- of Edinburgh , Session 1875-76. 35 gramme of lessons; there being capitation grants of money to the managers of these schools for scholars who, at the annual inspec- tions, pass satisfactory examinations in various branches of science. I have thus at some length explained what has been done during the last ten, and more particularly during the last five years, for increasing the means of scientific instruction in our universities, colleges, and even in elementary schools, because of the import- ant bearing of these measures in promoting such objects as this Society aims at. When vast multitudes of our population become conversant with science, who knew nothing of science before, who can doubt that investigation will be stimulated, and that discoveries and inventions will be made with a speed hitherto unprecedented ? But there is another measure of even greater importance to science, which is about to be taken in this country. Our schools, colleges, and universities are institutions for teaching truths, and explaining facts already known. It is now proposed to establish colleges of research, as they have heen called, for aiding in the discovery of truths, facts, and principles not yet known. In the year 1868, the British Association for the advancement of science appointed a committee of some of its most eminent members to report on the two following questions “Does there exist in the United Kingdom of Great Britain and Ireland, sufficient provision for the vigorous prosecution of physical research ?” “ If not, what farther provision is needed, and what measures should be taken to secure it” In the following year that committee gave in a report, answer- ing these questions thus : — “ The provision now existing in the United Kingdom is far from sufficient for the vigorous prosecution of physical research. “ Whilst greatly increased facilities for extending physical research are required, your committee do not consider it expedient to define how these facilities should be provided.” The committee added, that “ as the whole question of the relation of the State to Science is at present in a very unsatisfactory position, they urge that a Royal Commission alone is competent to deal with the subject.” 36 Proceedings of the Royal Society That report having been approved of by the Association, an influential deputation waited on Her Majesty’s G-overnment, to suggest the appointment of a Commission ; and accordingly in May 1870 such a Commission was appointed. This Commission has been most diligent in its investigation and discussion of the several points remitted to it. They have exa- mined several hundred witnesses, and have issued no less than eight reports. Besides ascertaining the condition of our universities, colleges, and endowed first-class schools, as regards their teaching power, and suggesting in many cases that assistance should be given to them by the State, the Commissioners took up the other important question, to which the British Association specially had called attention — viz. this, whether the State ought not to aid researches for discovering new scientific facts and truths. As the report of the Commissioners on this question is of great interest alike to men of science and to scientific bodies in this country, 1 quote a few sentences to show the opinion of these Koyal Commissioners, and the advice they give to Her Majesty’s Government : — (‘ The great advances in physical science which have been made in this country, and within this century, by such men as Dalton, Davy, and Faraday, without aid from the State; the existence of numerous learned societies ; and the devotion of some few rich individuals to the current work of science, at first sight appear to reduce the limits within which State aid to research is required in this country. “ But whilst we have reason to be proud of the contributions of some great Englishmen to our knowledge of the laws of nature, it must be admitted that at the present day scientific investigation is carried on abroad to an extent, and with a com- pleteness of organisation to which this country can offer no parallel. The work done in this country by private individuals, although of great value, is small when compared with that which is needed in the interests of science ; and the efforts of the learned societies, not excepting the Boyal Society, are directed merely to the dis- cussion and publication of the scientific facts brought under their 37 of Edinburgh, Sessio7i 1875-76. notice. These societies do not consider it any part of their corporate functions to undertake or conduct research. ..... “But whatever may be the disposition of individuals to conduct researches at their own cost, the advancement of modern science requires investigations and observations extending over areas so large, and periods so long, that the means and lives of nations are alone commensurate with them. “ Hence the progress of scientific research must in a great measure depend upon the aid of Governments. As a nation, we ought to take our share of the current scientific work of the world. Much of this work has always been voluntarily undertaken by individuals, and it is not desirable that Government should super- sede such efforts ; but it is bound to assume that large portion of the national duty, which individuals do not attempt to perform, or cannot satisfactorily accomplish.” The sentences which I have now read are the preamble and the basis of the conclusions to which the Commissioners unanimously came. These conclusions are as follows : — 1. “ The assistance given by the State in this country for the promotion of scientific research is inadequate; and it does not appear that the concession or refusal of assistance takes place upon sufficiently well-defined principles.” 2. “ More complete means are urgently required for scientific investigations, in connection with certain Government departments. Physical as well as other laboratories and apparatus for such in- vestigations ought to be provided.” 3. “ Important classes of phenomena relating to physical meteor- ology, and to terrestrial and astronomical physics, require observa- tions of such a character, that they cannot be advantageously carried on otherwise than under the direction of the Government .” 4. “ Whilst national collections of natural history are accessible to 'private investigators , it is desirable that they should be made still more useful for purposes of research than they are at present. We would now express the opinion that corresponding aid ought to be afforded to persons engaged in important physical and chemi- cal investigations ; and that, whenever practicable, such persons should be allowed access , under proper limitations, to such labora- tories as may be established or aided by the State.'1 38 Proceedings of the Royal Society 5. “ It has been tlie practice to restrict grants of money made to private investigators for purposes of research, to the expenditure actually incurred by them. We think that such grants might be considerably increased. We are also of opinion, that the restriction to which we have referred, however desirable as a general rule, should not be maintained in all cases, but that, under certain cir- cumstances and with proper safeguards, investigators should be remunerated for their time and labour. ” 6. “ The grant of L.1000 administered by the Eoyal Society, has contributed greatly to the promotion of research, and the amount of this grant may with advantage be considerably increased.’’ “In the case of researches which involve, and are of sufficient importance to deserve, exceptional expenditure, direct grants, in addition to the annual grant made to the Royal Society, should be made in aid of the investigations.” 7. “ The proper allocation of funds for research ; the establish- ment and extension of laboratories and observatories ; and generally, the advancement of science, and the promotion of scientific instruc- tion as an essential part of public education, would be most effec- tually dealt with, by a Ministry of Science and Education , and we consider the creation of such a ministry of primary importance .” 8. “ The various departments of the Government have from time to time referred scientific questions to the Council of the Royal Society for its advice. We believe that the work of a Minister of Science, even if aided by a well-organised scientific staff, and also the work of the other departments, would be materially assisted, if they were able to obtain, in all cases of exceptional importance or difficulty, the advice of a Council representing the scientific knowr- ledge of the nation.” 9. “ This Council should represent the chief scientific bodies in the United Kingdom. With this view, its composition need not differ very greatly from that of the present Government Grant Committee of the Royal Society. It might consist of men of science selected by the Council of the Royal Society, together with representatives of other important scientific societies, and a certain number of persons nominated by the Govenment.” Such, gentlemen, are the conclusions and recommendations of these Royal Commissioners on a subject deeply interesting not only of Edinburgh , Session 1875-76. 39 to all scientific bodies, and men of science in this country, but to the nation at large. The Commissioners are men eminently qualified by social position, by enlightened knowledge, and by a thorough investigation of the subject, to pronounce an opinion, and I feel very confident that when their report comes before Parliament, their conclusions will be accepted, the organisation recommended by them agreed to, and the necessary supplies ungrudgingly voted. I have, before concluding, only one other point to mention. No great measure, whether political or educational, can be adopted in this country by the G-overnment, or even by Parliament, which has not obtained previously the general assent of the community. Now it is a gratifying circumstance, that during the last few months, many distinguished men, good judges of public opinion, and who also themselves influence public opinion, have recently taken occasion to advert to the question of scientific instruction. I have already mentioned the names of His Royal Highness Prince Leopold and his Grace the Duke of Marlborough. It so happens that the same page of the “ Times” newspaper, of the 12th Nov., which reports what they said, gives speeches in the same direction by Sir Alexander Cockburn, Lord Chief- Justice of England, and by Mr Gladstone, the ex-Premier. Going back a few weeks, I find speeches by the Duke of Devonshire, the Marquis of Harting- ton, the Earl of Derby, the Marquis of Ripon, Lord Winmanleigh, Lord Frederick Cavendish, Sir Stafford Northcote, the Right Hon. Lyon Playfair, and Mr Bell, M.P. for Hartlepool, one of our most extensive and intelligent iron-masters. These names I mention to show that the great landowners of the country, and also many distinguished statesmen, are responding heartily to the appeal made to them by our manufacturers and merchants, who feel that their own interests, and the continued prosperity of the country in trade and commerce, require institu- tions which will give to their sons, and also to the working classes, a more technical education than they have hitherto received. With such combined action, who can doubt that an immense impetus will be given both to scientific teaching and to scientific research ? Wonderful indeed have been the discoveries during the last half century, even with the scanty appliances whicli men of science 40 Proceedings of the Royal Society have hitherto had at their command. These discoveries, the Lord Chief-Justice Cockburn said, “ perfectly overwhelmed him with astonishment,” and as the Royal Commissioners said, may justly invoke national pride, that so many of them should be due to the unaided efforts of individuals. What, then, may we look forward to in the next half century, with the additional appliances which these Commissioners recommend ? But, perhaps, here a word of caution, even from so humble an adviser as myself, may be allowed. Lord Chief- Justice Cockburn, on the occasion to which I have referred, says — “ No one bows with a more profound and reverent worship at the shrine of science than I do. No one values more than I do classical attainments. Nevertheless, allow me to say, that I know of no study more valu- able to an Englishman than the study of English. Nothing is more valuable than the power of English composition, English oratory, and English elocution; and greatly as I* value classical knowledge, and the knowledge of foreign languages, I still say, that the English language and English composition are of the first impor- tance to Englishmen.” These remarks he followed up by announcing his wish to give a prize of twenty guineas annually for a piece of English composition. Much to the same purpose, our distinguished colleague Mr Lyon Playfair, when assisting the other day to inaugurate the Science College at Leeds, expressed a hope that the institution would not be confined to science, but would embrace letters and the arts. These views suggest one danger to be avoided by those who are anxious to establish colleges and schools for scientific teaching. The country, willing as it undoubtedly is to supply deficiencies in this respect, will certainly not agree that a knowledge of science shall be all that a well-educated Englishman or Scotchman ought to possess. But there is another danger, and one more serious. Mr Glad- stone, when distributing the prizes of the science and art classes at Greenwich, three weeks ago, made these impressive remarks: — “ Whatever I may think of the pursuits of industry and science, and of the triumphs and glories of art, I do not mention any one of these things as the great specific for alleviating the sorrows of of Edinburgh, Session 1875-76. 41 human life, and meeting the evils which deface the world. I believe firmly in science and art, for their own purposes. I be- lieve in their reality, their efficacy, and their value ; I believe they are efficacious and valuable for the purposes for which they are ordained, but not for purposes for which they were not ordained. If I am asked what is the remedy for the deeper sorrows of the human heart — what a man should chiefly look to in his progress through life, with which to sustain him under trials nd affliction — I must point to something very different, to some- thing which in a well-known hymn is called ‘the old, old story/ It is this ‘ old, old story, told in a good old book, with the teaching to be found there, which is the greatest and best gift ever given to mankind, a gift carrying with it and imposing upon all alike, the most solemn trusts and responsibility, because arousing the fullest recollections of the past and the brightest hopes of the future. I venture upon this observation for myself, lest, in speak- ing of the immense value which is to be attached to the subjects with which we are dealing to-night, it should be supposed I was setting them up as having some exclusive right to allegiance upon your minds and hearts, or, at any rate, a right paramount to every other.” I much fear that this warning of the ex-Premier is needed. I fear it may be said, not merely of men of science, but of others also, that they often allow their hearts and minds to be so occupied — so engrossed with pursuits and studies, as to leave no room for other things which should find a place there also. Men of science have sometimes been charged, not merely with allowing their minds to be too much engrossed in this way, but with conceit and arrogance, engendered by the consciousness of possessing wisdom above the great bulk of their countrymen. The true man of science, is fairly amenable to no such charge. So far from possessing that “pride, and arrogance, and fro ward mouth,” which is condemned in the good old book referred to by Mr Glad- stone, be is , and at all events should he , the reverse of all this ; for whatever amount of knowledge he acquires, whatever the dis- coveries he achieves, no one sees so clearly the immensity of what still remains to be discovered. Even in our own planet, how little do we yet know of the composition of the earth’s interior, how VOL. IX. F 42 Proceedings of the Royal Society little of its deep oceans, how little of ne great atmosphere which surrounds us! And even if we knew and understood all and every part of our own habitation, what is that, when we think what a tiny atom that habitation is in the great system of the universe, seen and unseen! The true man of science, knowing all this, is humble-minded, not arrogant or supercilious; diffident, not presumptuous; forbear- ing, not intolerant. If these are the qualities which men of science possess and show, whilst prosecuting their studies and researches, they will secure favour for themselves and for their noble pursuits. They will be accepted and respected as the expounders of the grand and beautiful laws by which God governs the universe — laws , a know- ledge and a right application of which will assuredly conduce, alike to the prosperity of nations and to the happiness of the human race. The following statement in regard to the number of the present Fellows of the Society was laid on the table by the Secretary : — 1. Honorary Fellows — Royal Personage — His Royal Highness the Prince of Wales, . . 1 British Subjects — John Couch Adams, Esq., Cambridge; Sir George Biddell Airy, Greenwich; Thomas Andrews, M.D., Belfast (Queen’s College); Thomas Carlyle, Esq., London; Arthur Cayley, Esq., Cambridge; Charles Darwin, Esq., Down, Broomley, Kent; John An- thony Froude, Esq., London; James Prescott Joule, LL.D., Cliffpoint, Higher Broughton, Manchester; William Lassell, Esq., Liverpool; Rev. Dr Hum- phrey Lloyd, Dublin; William Hallowes Miller, LL.D., Cambridge; Richard Owen, Esq., London; Lieut. -General Edward Sabine, R.A., London; George Gabriel Stokes, Esq., Cambridge; James Joseph Sylvester, LL.D., London; William Henry Fox Talbot, Esq., Lacock Abbey, Wiltshire; Alfred Tennyson, Esq., Freshwater, Isle of Wight, . . 17 Carry forward, 18 of Edinburgh , Session 1875-76. Brought forward, Foreign — Claude Bernard, Paris; Adolphe Theodore Brong- niart, Paris: Robert Wilhelm Bunsen, Heidelberg; Michael Eugene Chevreul, Paris; James D. Dana, LL.D., Newhaven, Connecticut; Heinrich Wilhelm Dove; Jean Baptiste Dumas, Paris; Charles Dupin, Paris; Christian Gottfried Ehrenberg, Berlin; Elias Fries, Upsala; Herman Helmholtz, Berlin ; August Kekule, Bonn; Gustav Robert Kirchhoff, Heidel- berg ; Herman Kolbe, Leipzig ; Albert Kolliker, Wurzburg ; Ernst Edward Kummer, Berlin ; Johann von Lamont, Munich; Richard Lepsius, Berlin ; Rudolph Leuckart, Leipzig ; Urbain Jean Joseph Leverrier, Paris; Joseph Lionville, Paris ; Henry Milne-Edwards, Paris ; Theodore Mommsen, Berlin ; John Lothrop Motley, United States; Louis Pasteur, Paris; Professor Benjamin Peirce, United States Survey; Adolphe Pictet, Geneva; Henry Victor Regnault, Paris; Angelo Secchi, Rome ; Karl Theodor von Siebold, Munich; Bernard Studer, Berne; Otto Torell, Lund; Rudolph Virchow, Berlin; Wilhelm Eduard Weber, Gottingen; Friedrich Wohler, Gottingen, Total Honorary Fellows at March 1875, 18 35 The following Foreign Honorary Fellows were elected in March 1875 — Dove, Kekule, Kolbe, Kummer, Lionville, Motley. The following are the Honorary Fellows deceased during the year — Foreign — M. Comte de Remusat, ... 1 British — Sir Charles Lyell, Bart., Sir W. E. Logan, Sir Charles Wheatstone, 3 2. Non-resident Fellow under the Old Laws — Sir Richard Griffiths, .... Total Honorary and Non-resident Fellows, 6th Dec. 1875, 44 Proceedings of the Royal Society 3. Ordinary Fellows — Ordinary Fellows at November 1874, . . . . 345 New Fellows , 1874-75. — John Aitken, Esq. ; The Hon. James Bain ; Dr Ludwick Bernstein ; James Bryce, LL.D.; John Christie, Esq.; Robert Clark, Esq.; Dr T. S. Clonston ; Dr William Craig ; Daniel G. E. Eliot, Esq.; Thomas Fairley, Esq.; Robert Gray, Esq.; Sir John Hawkshaw; William Jack, Esq.; Archibald Kirk- wood, LL.D.; John Ramsay L’Amy, Esq.; C. H. Millar, Esq.; John Milroy, Esq.; E. W. Prevost, Esq.; Ralph Richardson, Esq.; Michael Scott, Esq.; James Syme, Esq.; James Thomson, LL.D.; Charles Wilson Vincent, Esq. ; Professor Daniel Wilson, .... 24 B. Baden Powell, formerly elected, but not admitted till 1874; Dr Alexander Wood (re-admitted), . 2 Total New Fellows, . . 26 371 Deduct Deceased. — Rev. Dr Aitken; John Auld, Esq.; Dr J. Hughes Bennet ; Rev. Dr Crawford ; Col. Seton Guthrie; Sir William Jardine,Bart. ; Professor Macdonald; Hon. Lord Mackenzie; E. Meldrum, Esq.; Ven. Arch- deacon Sinclair, 10 Resigned. — Rev. Thomas M. Lindsay ; John L. Douglas Stewart, Esq., . . ... 2 Cancelled. — Charles Lawson, Esq., .... 1 33 Total number of Ordinary Fellows at November 1874, . 358 Add Honorary and Non-Resident Fellows, ... 50 Total Ordinary and Honorary Fellows at commencement of Session 1875 (6th December), 408 The following Communication was read : — The Volcanic Eruptions of Iceland in 1874 and 1875. By Captain Burton. (With two Maps of Iceland). Shortly after reading “Volcanic Eruptions in Iceland” (the “ Scotsman,” May 21), and “ An Appeal for Iceland ” (the “Times” July 1), I made a trip to Arctis, partly with a view of inspecting and inquiring into the last outbreaks. Perhaps your energetic Society may not be unwilling to have an unprejudiced account of what was seen and heard. N° 1,2,3, Eru M'Swlane Si Eis'idine . LiiH? Efe? Eruption 29 tK March 1875. N° 1,2,3, Eruptions with intermissions during the years 1867,1869, 1870-72. N° 4, Eruption about Christmas 1874. U? 5. Eruption 29 March 1875. The brown shading mark the Ashes thrown S.E. to East. "William P Nimmo, London 4 Edint>ur£h William E "Nrmmo, London Sc. Edinburgh Dttsilbss - Skplualr indirect mllet From Tyre)'/ M'y- r thro a dJudl tonp low snowy dew i Ik. '“^ViS leant? said to ha.fi been seen- Prom nd. supposed, cause oP Veru/jord, Pop Re,v* Siouriur Gurinarson places it "Lone. (G.) 30 ° 20. | Vaj,U4ui4t ^ William P "Nimmo, London . five, in the second for three, and in the third for four hours. The layer of pumice and ashes measured some 4J inches deep in the Jokulsdal, and 1J in the Seyfiisfjorb. This was the sixth explosion since the outbreak, and about every tenth or twelfth day the violence increased. The line extended through the Od&fiahraun to a little north of Reykjahlifi-Grimstafiir- road. About Easter-day a thick smoke was seen at Mofirudal a Fjollum ; it rose south of Herfiubreifi, and many erroneously thought that it came from Mofirufialsland. Others supposed it to rise from the Dyngjufjoll, but it was certainly from Yatnajdkull, or from the Tungu (Boab or Mesopotamia), formed by the westermost forks of the Jokulsa. The discharge of pumice ( Danice u Pimpsteen ”) was so abundant that for days the ferry boats could not cross the stream. The “ Norbanfari ” of May 13 contains an unsigned article, bringing up the account of our My-vatn eruption to May 5. Loud thunderings with thick smoke were noticed on the last “ Tuesday in the winter,” that is, on April 13; the summer beginning with “ Sumarm&l,” April 17. On the “ first summer day ” (April 22) four men took horse to visit the volcano. From Kollottafjall they saw a fiery crevasse, made like a mountain u fjargyd,” or sheep fissure where the animals take refuge during bad weather; and on the borders of the SveinagjA, where a fine grassy plain formerly extended, they found a high hill of lava pierced with three craters lying on a meridian. These vents roared loudly, and threw up rocks, which returned to the earth after 45 seconds. The smaller rapilli rising like smoke disappeared in the air, and presently fell like snow. From the largest focus, which lay south of the road, a fiery flood ran westward : it had been reported three (Danish) miles long, but it proved to be about 1000 fathoms, with a breadth of 300 to 400. The people of My-vatnssveit have lost a little grass, chiefly to the north of the road, and their ponies may suffer during the winter. Some convulsion has taken place in the Dyngjufjoll, whence, for a long time, more smoke issued than during the winter. There was a great eruption close to the Od4<5a- liraun on March 18 and 19, and the concussion of the air drove the farm peeple from their beds. On March 23 fire was reported to have proceeded from forty places lying close to the Holsfjoll road, but it lay west, not east, of the Jokulsa. 56 Proceedings of the Royal Society Extracts from the letter of my friend, Sira Sigurftur Gunnarsson, the priest of Hallormsta'S, addressed to the “ Norftanfari ” of April 24, appeared in the “ Times ” of July 1, 1875. It is dated March 29, 1875, and headed “ Fall of Pumice and Ashes in Mulasyla.” The author, I may remark, has more than once visited the Vatna- jokull. The following interesting details may be added to the abstract : — “ During the Yule of 1873, and in early 1874, an earth- quake shook the eastern regions, after which the people of the Fjoll country saw two tall pillars of thick smoke apparently proceeding from the Askja or Dyngjufjoll; and viewed from Hallormsta<5arh&ls they rose at a considerable distance from each other. Early in the year there was no fire in the My-vatnsoroefi, and the earthquake became less violent towards the end of the winter. ” After noticing the thunderings and the ash and pumice rain of March 29 (Easter Monday) reported in the “ Times,” my reverend friend continues : — “ The movement appears to have taken place in the southern part of the Dyngjufjoll, westward of Herftubreift, and a short way north of the winter Grjd. The direction of the ashes was on both sides of a line to Modrudal and Fossvellir, as far as the Undos in Hjaltarstaftarthingd and the Vatnsdalsfjall. Another shower, travelling from west to east, and extending four (Danish) miles, fell at Bru, and a mile and a half east of Aftalbol (Rrafnkelsdal), Kleif (Fljotsdal), Skriftdal, and as far as Fdskrufts- fjorft to the south-east. The amount which fell east of that line in Breiftdal and Stoftvarfjorft was trifling. If we draw one straight line from the focus of the eruption eastward between Fdskrufts and Stoftvarfjorft, and a second from Vatnsdalsfjall near Njarftvik, also to the east, the area upon which the ashes and pumice rained would hardly be less than 100 square miles. Also assuming the average depth of the layer at 3 inches, we must assign to the discharge of March 19 a weight of 3840 tons.” “It is reported that the ash showers have ruined twenty farms in the Jokulsdal (between the Lagarfljot and the eastern Jokulsa) and in the northern Mula Sysla, where the owners are preparing to abandon their property. The position of the Fljotsdalsherad, where the scoriaceous rains fell thickest, are the Jokulsdal, Fell, Fljostdal, Skogar, SkriSdal, Vellir, and EySathinghA Heavy and terrible showers also desolated Norftfjorti, Reyftarfjorft, Myvafjorft, and 57 of Edinburgh, Session 1875-7G. LoftmundarfjoriS. Where the land has abundance of water, as in parts of SkriSdal, Vellir, and EySathinghd, the farmers hope that the ashes will disappear during the spring, and that they will be dissolved by the rains.” This interesting letter concludes with an exhortation “ not to abandon the holdings for good,” and with excellent advice about the measures to be taken. Yet it owns that “ from this fearful visitation all husbandry in the east country must come to utter ruin,” and the less Icelanders are advised not to emigrate the better for the island. The writer of “An Appeal for Iceland” (“Times,” July 1, 1875), compares this mild and harmless eruption, which has not destroyed a single life, with the terrible convulsions of 1783, which killed some 14,000 human beings. He also calculates the destruc- tion of pastures to the extent of 2500 to 3000 square miles, while popular computations make 4000 square miles the habitable area of Iceland. According to PHI PHs^on only four farms on the west of the Jokulsd have suffered severely. These are, going from south to north, Bru, EyrikstaSir, H&konarstaSir, and Arndrstaftir. Ilerra Thorftur Grudjonsson, factor at Husavik, never even heard of the eruption till I showed .him the nepawspers. Finally, the brown shadings in my chart, marking the eastern and north-eastern limits of the ash showers, and copied from an Iceland map obligingly lent to me by my friend, Mr Hubert Mackay Smith, may be allowed to prove that the damage extends over a small area. Mr Jon A. Hjaltalln, of the Advocate’s Library, Edinburgh, received (June 26) trustworthy accounts of the ash and pumice rain. “ It extended over several parts of Norftur Mulasysla and SucSur Mulasysla, depositing a layer about 1J inches thick. In some places the winds have carried it off, but sundry parishes will be unable to keep their live stock at home this summer. Next hot season, however, it is expected that the pastures will be all right.” Mr W. L. Watt, who has just ridden over the ground, found the pumice and ashes beginning about the middle course of the Svarti, (N. lat. 64° 50'), and extending northwards to Her'SubreitS (65° 10'). or a total depth of 20 to 25 miles, bounded eastward by the Jokulsa, where the country is not, and never has been, habited by man. VOL. IX. n 58 Proceedings of the Royal Society. The limits of this paper do not permit me to enter into all the details of the last eruption in Iceland ; but the reader may be assured that the outline and the main features of the subject are correctly drawn. The following Gentlemen were elected Fellows of the Society: — Bruce Ailan Bremner, M.D. Rev. Francis Edward Belcombe. PROCEEDINGS OF THE ROYAL SOCIETY OF EDINBURGH. vol. ix. 1875-76. No. 91. Ninety-Third Session. Monday , 2CBA December 1875. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. Yortex Statics. By Sir William Thomson. (Abstract.) The subject of this paper is steady motion of vortices. 1. Extended definition of “steady motion.” The motion of any system of solid or fluid or solid and fluid matter is said to be steady when its configuration remains equal and similar, and the velocities of homologous particles equal, however the configuration may move in space, and however distant individual material particles may at one time be from the points homologous to their positions at another time. 2. Examples of steady and not steady motion (1.) A rigid body symmetrical round an axis, set to rotate round any axis through its centre of gravity, and left free, performs steady motion. Not so a body having three unequal principal moments of inertia. (2.) A rigid body of any shape, in an infinite homogeneous liquid, rotating uniformly round any, always the same, fixed line, and moving uniformly parallel to this line, is a case of steady motion. (3.) A perforated rigid body in an infinite liquid moving in the VOL. ix. i 60 Proceedings of the Boyal Society manner of example (2.), and having cyclic irrotational motion of the liquid through its perforations, is a case of steady motion To this case belongs the irrotational motion of liquid in the neigh bourhood of any rotationally moving portion of fluid of the same shape as the solid, provided the distribution of the rotational mo tion is such that the shape of the portion endowed with it remains unchanged. The object of the present paper is to investigate general conditions for the fulfilment of this proviso ; and to inves tigate, farther, the conditions of stability of distribution of vortex motion satisfying the condition of steadiness. 3. General synthetical condition for steadiness of vortex motion. — The change of the fluid’s molecular rotation at any point fixed in space must be the same as if for the rotationally moving portion of the fluid were substituted a solid, with the amount and direction of axis of the fluid’s actual molecular rotation inscribed or marked at every point of it, and the whole solid, carrying these inscrip- tions with it, were compelled to move in some manner answering to the description of example (2). If at any instant the distribu- tion of molecular rotation * through the fluid, and corresponding distribution of fluid velocity, are such as to fulfil this condition, it will be fulfilled through all time. 4. General analytical condition for steadiness of vortex motion. — If, with (§ 24, below) vorticity and “ impulse,” given, the kinetic energy is a maximum or a minimum, it is obvious that the motion is not only steady, but stable. If, with same conditions, the energy is a maximum-minimum, the motion is clearly steady, but it may be either unstable or stable. 5. The simple circular Helmholtz ring is a case of stable steady motion, with energy maximum-minimum for given vorticity and given impulse. A circular vortex ring, with an inner irrotational annular core, surrounded by a rotationally moving annular shell (or endless tube), with irrotational circulation outside all, is a case of motion which is steady, if the outer and inner contours of the * One of the Helmholtz’s now well-known fundamental theorems shows that, from the molecular rotation at every point of an infinite fluid the velocity at every point is determinate, being expressed synthetically by the same formulae as those for finding the “ magnetic resultant force” of a pure electro-magnet. ■ — Thomson’s Reprint of Papers on Electrostatics and Magnetism. 61 of Edinburgh, Session 1875-76. section of the rotational shell are properly shaped, but certainly unstable if the shell be too thin. In this case also the energy is maximum-minimum for given vorticity and given impulse. 6. In these examples of steady motion, the “ resultant impulse” (V. M.* § 8) is a simple impulsive force, without couple; the cor- responding rigid body of example 3 is a circular toroid, and its motion is purely translational and parallel to the axis of the toroid. 5. We have also exceedingly interesting cases of steady motion in which the impulse is such that, if applied to a rigid body, it would be reducible, according to Poinsofs method, to an impulsive force in a determinate line, and a couple with this line for axis. To this category belong certain distributions of vorticity giving longitudinal vibrations, with thickenings and thinnings of the core travelling as waves in one direction or the other round a vortex ring, which will be investigated in a future communication to the Koyal Society. In all such cases, the corresponding rigid body of § 2 example (2) has both rotational and translational motion. 7. To find illustrations, suppose, first, the vorticity (defined below, § 24) and the force resultant of the impulse to be (according to the conditions explained below, § 29) such that the cross section is small in comparison with the aperture. Take a ring of flexible wire (a piece of very stout lead wire with its ends soldered together answers well), bend it into an oval form, and then give it a right-handed twist round the long axis of the oval, so that the curve comes to be not in one plane (fig. 1). A properly-shaped twisted ellipse of this kind [a shape perfectly determinate when the vorticity, the force resultant of the impulse, and the rotational moment of the impulse (V. M. § 6), are all given] is the figure of the core in what we may call the first f steady mode of single and simple toroidal * My first series of papers on vortex motion in the “ Transactions of the Royal Society of Edinburgh,” will he thus referred to henceforth. t First or gravest, and second, and third, and higher modes of steady mo- tion to be regarded as analogous to the first, second, third, and higher funda- mental modes of an elastic vibrator, or of a stretched cord, or of steady undulatory motion in an endless uniform canal, or in an endless chain of mutually repulsive links. 62 Proceedings of the Iioyal Society vortex motion with rotational moment. To illustrate the second steady mode, commence with a circular ring of flexible wire, and pull it out at three points, 120° from one another, so as to make it into as it were an equilateral triangle with rounded corners. G-ive now a right-handed twist, round the radius to each corner, to the plane of the curve at and near the corner; and, keeping the cha- racter of the twist thus given to the wire, bend it into a certain determinate shape proper for the data of the vortex motion. This is the shape of the vortex core in the second steady mode of single and simple toroidal vortex motion with rotational moment. The third is to be similarly arrived at, by twisting the corners of a square having rounded corners ; the fourth, by twisting the corners of a regular pentagon having rounded ‘corners ; the fifth, by twisting the corners of a hexagon, and so on. In each of the annexed diagrams of toroidal helixes a circle is introduced to guide the judgment as to the relief above and depression below the plane of the diagram which the curve repre- sented in each case must be imagined to have. The circle may be imagined in each case to be the circular axis of a toroidal core on which the helix may be supposed to be wound. To avoid circumlocution, I have said, “give a right-handed twist ” in each case. The result in each case, as in fig. 1, illus- trates a vortex motion for which the corresponding rigid body describes left-handed helixes, by all its particles, round the central axis of the motion. If now, instead of right-handed twists to the plane of the oval, or the corners of the triangle, square, pentagon, &c., we give left-handed twists, as in figs. 2, 3, 4, the result in each case will be a vortex motion for which the corresponding rigid body describes right-handed helixes. It depends, of course, on the relation between the directions of the force resultant and couple resultant of the impulse, with no ambiguity in any case, whether the twists in the forms, and in the lines of motion of the corresponding rigid body, will be right-handed or left-handed. 8. In each of these modes of motion the energy is a maximum- minimum for given force resultant and given couple resultant of impulse. The modes successively described above are successive solutions of the maximum-minimum problem of § 4; a determinate problem with the multiple solutions indicated above, but no other of Edinburgh, Session 1875-76. 63 solution, when the vorticity is given in a single simple ring of the liquid. 9. The problem of steady motion, for the case of a vortex line with infinitely thin core, bears a close analogy to the following purely geometrical problem : — Find the curve whose length shall be a minimum with given resultant projeetional area, and given resultant areal moment (§ 27 below). This would be identical with the vortex problem if the energy of an infinitely thin vortex ring of given volume and given cyclic constant were a function simply of its apertural circum- ference. The geometrical problem clearly has multiple solutions answering precisely to the solutions of the vortex problem. 10. The very high modes of solution are clearly very nearly identical for the two problems (infinitely high modes identical) and are found thus : — Take the solution derived in the manner explained above, from a regular polygon of N sides, when N is a very great number. It is obvious that either problem must lead to a form of curve like that of a long regular spiral spring of the ordinary kind bent round till its two ends meet, and then having its ends properly cut and joined so as to give a continuous endless helix with axis a circle (instead of the ordinary straight line-axis), and N turns of the spiral round its circular axis. This curve I call a toroidal helix, because it lies on a toroid * just as the common regular helix lies * 1 can a circular toroid a simple ring generated by the revolution of any singly-circumferential closed plane curve round any axis in its plane not cutting it. A “tore,” following French usage, is a ring generated by the revolution of a circle round any line in its plane not cutting it. Any simple 64 Proceedings of the Royal Society on a circular cylinder. Let a be the radius of the circle thus formed by the axis of the closed helix ; let r denote the radius of the cross section of the ideal toroid on the surface of which the helix lies, supposed small in comparison with a; and let 0 denote the inclination of the helix to the normal section of the toroid. We have ~ 27 ra a taD 6 = NlSn7 = Nr ’ because is as it were the step of the screw, and 2ttt is the cir- cumference of the cylindrical core on which any short part of it may be approximately supposed to be wound. Let k be the cyclic constant, I the given force resultant of the impulse, and /x the given rotational moment. We have (§ 28) approximately Hence I — - K7ra2, /x = KN7rr2a . \J K7r’ \f Nk^ttHs ’ = /i. \/ N/XK57T5 tan 6 11. Suppose, now, instead of a single thread wound spirally round a toroidal core, we have two separate threads forming as it were a “ two-threaded screw,” and let each thread make a whole ring, or any solid with a single hole through it, may be called a toroid ; but to deserve this appellation it had better be not very unlike a tore. The endless closed axis of a toroid is a line through its substance passing somewhat approximately through the centres of gravity of all its cross sec- tions. An apertural circumference of a toroid is any closed line in its surface once round its aperture. An apertural section of a toroid is any section by a plane or curved surface which would cut the toroid into two separate toroids. It must cut the surface of the toroid in just two simple closed curves, one of them completely surrounding the other on the sectional surface : of course, it is the space between these curves which is the actual section of the toroidal substance, and the area of the inner one of the two is a section of the aperture. A section by any surface cutting every apertural circumference, each once and only once, is called a cross section of the toroid. It consists essentially of a simple closed curve. 65 of Edinburgh, Session 1875-76. number of turns round the toroidal core. The two threads, each endless, will be two helically tortuous rings linked together, and will constitute the core of what will now be a double vortex ring. The formulae just now obtained for a single thread would be appli- cable to each thread, if k denoted the cyclic constant for the circuit round the two threads, or twice the cyclic constant for either, and N the number of turns of either alone round the toroidal core. But it is more convenient to take N for the number of turns of both threads (so that the number of turns of one thread alone is JN), and k the cyclic constant for either thread alone, and thus for very high steady modes of the double vortex ring I = 2/c7ra2, fx = KN7rr2a, tan 0 = 11 sj N m N/XK^7r5 * Lower and lower steady modes will correspond to smaller and smaller values of N, but in this case, as in the case of the single vortex core, the form will be a curve of some ultratranscendent character, except for very great values of N, or for values of 6 in- finitely nearly equal to a right angle (this latter limitation leading to the case of infinitely small transverse vibrations). 12. The gravest steady mode of the double vortex ring corre- sponds to N = 2. This with the single vortex core gives the case of the twisted ellipse (§ 7). With the double core it gives a sys- tem which is most easily understood by taking two plane circular rings of stiff metal linked together. First, place them as nearly coincident as their being linked together permits (fig. 5). Then separate them a little, and incline their planes a little, as shown in the diagram. Then bend each into an unknown shape deter- mined by the strict solution of the transcendental problem of analysis to which the hydro-kinetic investigation leads for this case. 13. Go back now to the supposition of § 11, and alter it to this : — 66 Proceedings of the Royal Society Let each thread make one turn and a half, or any odd num- ber of half turns, round the toroidal core : thus each thread will have an end coincident with an end of the other. Let these coincident ends he united. Thus there will he but one endless thread making an odd number N of turns round the toroidal core. The cases of N = 3 and N = 9 are represented in the annexed diagrams (fig. 9).* Imagine now a three-threaded toroidal helix, and let N denote the whole number of turns round the toroidal core, we have I = 3/<7ra2, fji = kN irr2a , tan 6 = Suppose now N to be divisible by 3 : then the three threads form three separate endless rings linked together. The case of N = 3 is illustrated by the annexed diagram (fig. 6), which is repeated from the diagram of Y. M. § 58. If N be not divisible by 3, the three threads run together into one, as illustrated for the case of N = 11 in the annexed diagram (fig. 7). 14. The irrotational motion of the liquid round the rotational cores in all these cases is such that the fluid velocity at any point is equal to, and in the same direction as, the resultant magnetic force at the corresponding point in the neighbourhood of a closed gal- * The first of these was given in § 68 of my paper on vortex motion. It has since become known far and wide by being seen on the back of the “ Unseen Universe.” of Edinburgh, Session 1875-76. 67 vanic circuit, or galvanic circuits, of the same shape as the core or cores. The setting forth of this analogy to people familiar, as modern naturalists are, with the distribution of magnetic force in the neighbourhood of an electric circuit, does much to promote a clear understanding of the still somewhat strange fluid motions with which we are at present occupied. 15. To understand the motion of the liquid in the rotational core itself, take a piece of Xndian-rubber gas-=pipe stiffened internally with wire in the usual manner, and with it construct any of the forms with which we have been occupied, for instance the sym- metrical trefoil knot (fig. 8, § 13), unit- ing the two ends of the tube carefully by tying them firmly by an inch or two of straight cylindrical plug, then turii the tube round and round, round its sinuous axis. The rotational motion of the fluid vortex core is thus represented. But it must be remembered, that the outer form of the core has a motion per- pendicular to the plane of the diagram, and a rotation round an axis through the centre of the diagram, and perpendicular to the plane in each of the cases represented by the preceding diagrams. The whole motion of the fluid, rotational and irrotational, is so related in its different parts to one another, and to the translational and rotational motion of the shape of the core, as to be everywhere slipless. 16. Look to the preceding diagrams, and, thinking of what they represent, it is easy to see that there must be a determinate parti- cular shape for each of them which will give steady motion, and I think we may confidently judge that the motion is stable in each, provided only the core is sufficiently thin. It is more easy to judge of the cases in which there are multiple sinuosities by a synthetic view of them (§ 3) than by consideration of the maxi- mum-minimum problem of § 8. 17. It seems probable that the two- or three- or multiple- threaded toroidal helix motions cannot be stable, or even steady, unless I, fx, and N are such as to make the shortest distances between different positions of the core or cores considerable in VOL. IX. K 68 Proceedings of the Poyal Society comparison with the core’s diameter. Consider, for example, the simplest case (§ 12, fig. 5) of two simple rings linked together. 18 Gro back now to the simple circular Helmholtz ring. It is clear that there must be a shape of absolute maximum energy for given vorticity and given impulse, if we introduce the restriction that the figure is to be a figure of revolution, that is to say, symmetrical round a straight axis. If the given vorticity be given in this determinate shape the motion will be steady, and there is no other figure of revolution for which it would be steady (it being understood that the impulse has a single force resultant without couple) . If the given impulse, divided by the cyclic constant, be very great in comparison with the two-thirds power of the volume of liquid in which the vorticity is given, the figure of steadiness is an exceedingly thin circular ring of large aperture and of approximately circular cross section. This is the case to which chiefly attention is directed by Helmholtz. If, on the other hand, the impulse divided by the cyclic constant be very small compared with the two-thirds power of the volume, the figure becomes like a long oval, bored through along its axis of revolution and with the ends of the bore ' rounded off for trumpeted) symmetrically, so as to give a figure something like the handle of a child’s skipping-rope, but sym- metrical on the two sides of the plane through its middle perpendicular to its length. It is certain that, however small the impulse, with given vorticity the figure of steadiness thus indicated is possible, however long in the direction of the axis and small in diameter perpendicular to the axis and in aperture it may be. I cannot, however, say at present that it is certain that this possible steady motion is stable, for there are figures not of revolution, deviating infinitely little from it, in which, with the same vorticity, there is the same impulse and the same energy, and consideration of the general character of the motion is not reassuring on the point of stability when rigorous demon- stration is wanting. 19. Hitherto I have not indeed succeeded in rigorously demon- strating the stability of the Helmholtz ring in any case. With given vorticity, imagine the ring to be thicker in one place than in another. Imagine the given vorticity, instead of being distributed in a symmetrical circular ring, to be distributed in a ring still, of Edinburgh, Sessio7i 1875-76. 69 with a circular axis, but thinner in one part than in the rest. It is clear that with the same vorticity, and the same impulse, the energy with such a distribution is greater that when the ring is symmetrical. But, now let the figure of the cross section of the ring, instead of being approximately circular, be made considerably oval. This will diminish the energy with the same vorticity and the same impulse. Thus, from the figure of steadiness we may pass continuously to others with same vorticity, same impulse, and same energy. Thus, we see that the figure of steadiness is, as stated above, a figure of maximum-minimnm, and not of abso- lute maximum, nor of absolute minimum energy. Hence, from the maximum-minimum problem we cannot derive proof of stability. 20. The known phenomena of steam rings and smoke rings show us enough of, as it were, the natural history of the subject to convince us beforehand that the steady configuration, with ordinary proportions of diameters of core to diameter of aperture, is stable, and considerations connected with what is rigorously demonstrable in repect to stability of vortex columns (to be given in a later communication to the Koyal Society) may lead to a rigorous demonstration of stability for a simple Helmholtz ring if of thin enough core in proportion to diameter of aperture. But at present neither natural history nor mathematics gives us perfect assurance of stability when the cross section is considerable in proportion to the area of aperture. 21. I conclude with a brief statement of general propositions, definitions, and principles used in the preceding abstract, of which some appeared in my series of papers on vortex motion com- municated to the Royal Society of Edinburgh in 1867-68 and 69, and published in the Transactions for 1869. The rest will form part of the subject of a continuation of that paper, which I hope to communicate to the Royal Society before the end of the present session. Any portion of a liquid having vortex motion is called vortex core, or, for brevity, simply “ core.” Any finite portion of liquid which is all vortex -core, and has contiguous with it over its whole boundary ir rotation ally moving liquid, is called a vortex . A vortex thus defined is essentially a ring of matter. That it must 7 0 Proceedings of the Royal Society be so was first discovered and published by Helmholtz. Some- times the word vortex is extended to include irrotationally moving | liquid circulating round or moving in the neighbourhood of vortex core ; but as different portions of liquid may successively come into the neighbourhood of the core, and pass away again, while the core always remains essentially of the same substance, it is more proper to limit the substantive term a vortex as in the definition I have given. 22. Definition I. — The circulation of a vortex is the circulation [V.M. § 60 (a)] in any endless circuit once round its core. What- ever varied configurations a vortex may take, whether on account of its own unsteadiness (§ 1 above), or on account of disturbances by other vortices, or by solids immersed in the liquid, or by the solid boundary of the liquid (if the liquid is not infinite), its “ circulation ” remains unchanged [V. M. § 59, Prop. (1)]. The circulation of a vortex is sometimes called its cyclic constant. Definition II. — An axial line through a fluid moving rotation- ally, is a line (straight or curved) whose direction at every point coincides with the axis of molecular rotation through that point [V. M. § 59 (2)]. Every axial line in a vortex is essentially a closed curve, being of course wholly without a vortex. 23. Definition III. — A closed section of a vortex is any section of its core cutting normally the axial line through every point of it. Divide any closed section of a vortex into smaller areas ; the axial lines through the borders of these areas form what are called vortex tubes. I shall call (after Helmholtz) a vortex filament any portion of a vortex bounded by a vortex tube (not necessarily infinitesimal). Of course, a complete vortex may be called therefore a vortex filament ; but it is generally convenient to apply this term only to a part of a vortex as just now defined. The boundary of a complete vortex satisfies the definition of a vortex tube. A complete vortex tube is essentially endless. In a vortex filament infinitely small in all diameters of cross sections “ rota- 71 of Edinburgh, Session 1875-76. tion varies [Y. M. § 60 (e)] from point to point of the length of the filament, and from time to time inversely as the area of the cross section. The product of the area of the cross section into the rotation is equal to the circulation or cyclic constant of the filament. 24. Vorticity will be used to designate in a general way the distribution of molecular rotation in the matter of a vortex. Thus, if we imagine a vortex divided into a number of infinitely thin vortex filaments, the vorticity will be completely given when the volume of each filament and its circulation, or cyclic constant, are given; but the shapes and positions of the filaments must also be given in order that, not only the vorticity, but its distribution, can be regarded as given. 25. The vortex density at any point of a vortex is the circula- tion of an infinitesimal filament through this point divided by the volume of the complete filament. The vortex density remains always unchanged for the same portion of fluid. By definition it is the same all along any one vortex filament. 26. Divide a vortex into infinitesimal filaments inversely as their densities so that their circulations are equal; and let the circula- tion of each be — of unity. n Take the projection of all the fila- ments on one plane. — of the sum of the areas of these projections n is (Y. M. §§ 6, 62) equal to the component impulse of the vortex perpendicular to that plane. Take the projections of the filaments on three planes at right angles to one another, and find the centre of gravity of the areas of these three sets of projections. Bind, according to Poinsot’s method, the resultant axis, force, and couple of the three forces equal respectively to — of the sums of the areas, and acting in lines through the three centres of gravity perpendicular to the three planes. This will be the resultant axis ; the force resultant of the impulse, and the couple resultant of the vortex. The last of these, that is to say, the couple is also called the rotational moment of the vortex (V. M. § 6). 72 Proceedings of the Royal Society 27. Definition IV. — The moment of a plane area round any axis is the product of the area multiplied into the distance from that axis of the perpendicular to its plane through its centre of gravity. Definition V. — The area of the projection of a closed curve on the plane for which the area of projection is a maximum will be called the area of the curve, or simply the area of the curve. The area of the projection on any plane perpendicular to the plane of the resultant area is of course zero. Definition VI. — The resultant axis of a closed curve is a line through the centre of gravity, and perpendicular to the plane of its resultant area. The resultant areal moment of a closed curve is the moment round the resultant axis of the areas of its pro- jections on two planes at right angles to one another, and parallel to this axis. It is understood, of course, that the areas of the projections on these two planes are not evanescent generally, except for the case of a plane curve, and that their zero values are generally the sums of equal positive and negative portions. Thus their moments are not in general zero. Thus, according to these definitions, the resultant impulse of a vortex filament of infinitely small cross section and of unit circulation is equal to the resultant area of its curve. The resultant axis of a vortex is the same as the resultant axis of the curve, and the rotational moment is equal to the resultant areal moment of the curve. 28. Consider for a moment a vortex filament in an infinite liquid with no disturbing influence of other vortices, or of solids, immersed in the liquid. We now see from the constancy of the impulse (proved generally in Y. M. § 19) that the resultant area, and the resultant areal moment of the curve formed by the filament, remain constant, however its curve may become con- torted ; and its resultant axis remains the same line in space. Hence, whatever motions and contortions the vortex filament may experience, if it has any motion of translation through space this motion must be on the average along the resultant axis. i of Edinburgh, Session 1875-76. 73 29. Consider now the actual vortex made up of an infinite number of infinitely small vortex filaments. If these be of volumes inversely proportional to their vortex densities (§ 25), so that their circulations are equal, we now see from the constancy of the impulse that the sum of the resultant areas of all the vortex filaments remains constant ; and so does the sum of their rotational moments: and the resultant areal axis of them all regarded as one system is a fixed line in space. Hence, as in the case of a vortex filament, the translation, if any, through space is on the average along its resultant axis. All this, of course, is on the supposition that there is no other vortex, and no solid immersed in the liquid, and no bounding surface of the liquid near enough to produce any sensible influence on the given vortex. 2. Experiments illustrating Rigidity produced by Centrifugal Force. By John Aitken, Esq. If an endless chain is hung over a pulley and the pulley driven at a great velocity, it is well known that the motion so communi- cated to the chain has almost no tendency to change the form of the curve in which the chain hangs, and that the principal effect of the motion is to confer on the chain a quasi-rigidity which enables it to resist any force tending to alter its curvature. This is only true in a general sense, and possibly may be true of some ideal form of chain ; but in all chains we can experiment on there are forces in action in the moving chain which tend to cause the chain to depart from the form which it has while at rest. I shall refer to these disturbing forces later on. As the disturb- ing forces in most chains are very small, we shall neglect them, and for the present suppose the centrifugal force just balances the tension at all points. The following experiments were made to illustrate the balance of these forces, to show that into whatever curves we may bend the chain when in motion, the centrifugal force has no tendency to alter these curves: that all forms are forms of stability, as far as the centrifugal force is concerned. The first experiments were to show the effect of destroying the balance between the tension and the centrifugal force. In these experiments the links on the descending side of the loop were 74 Proceedings of the Royal Society allowed to fall on a platform, so that part of the chain lay loose on the platform, thus destroyed the tension produced by the centrifugal force at the lower part of the chain. The chain was made to take the same velocity as the driving pulley, by being pressed into contact with it by means of an elastic wheel. I. When the chain was pressed at the point where it leaves the pulley there was no alteration in the path of the chain, because the chain after it leaves the pulley is moving in a straight line, and as there is no deviating force, there is no centrifugal force, and therefore, removing the tension in the chain has no effect on the direction of the motion of the links. II. When the chain was pressed at a point a little higher up the pulley, then the centrifugal force of the curved part of the chain resting on the pulley at the descending side, being unba- lanced by the tension, rises from the pulley, and is shot in a direc- tion away to one side of the pulley. Of course the curved part of the chain on the other side of the pulley has also a tendency to rise, but is kept in its place by the tension produced by putting the chain in motion after being stopped by the platform. III. When the chain is pressed on the ascending side of the pulley, then the chain rises up off the pulley and forms itself into a somewhat irregular curve resting on the platform, and touching the pulley at only one point. When the velocity is sufficient to raise it to a certain height, the conditions become altered. The chain in rising takes up all the slack chain lying on the platform, and a tension is produced in the chain by the centrifugal force, and unless we keep increasing the speed of the chain, it can no longer keep in its elevated position, because the centrifugal force is now balanced by the tension, and as the force of gravitation is now unbalanced, it gradually flattens the curve till the chain again comes to rest on the top of the pulley and spreads itself out in an irregular curve on the platform. IV. At the beginning of the previous experiment the centrifugal force being unbalanced by the tension, it overcomes the force of gravitation and causes the chain to rise into the air. After all the slack chain has been taken up, and a tension is produced in the chain by the centrifugal force, then the centrifugal force is balanced by the tension and is no longer capable of opposing gravitation, and 75 of Edinburgh , Session 1875-76. the chain begins to fall; but at this point its fall may be stopped, or the chain may be made to rise again by destroying the tension at the lower part of the chain. If we cause the chain, instead of meeting the platform at an acute angle, to strike it as near as pos- sible at right angles, then the motion of the chain where it strikes the platform is partly destroyed, and the chain again rises and may be kept balanced for a long time resting on the platform, and only touching the driving wheel at one point. The reason for this being, that if we partially stop the motion of the links by causing them to strike the platform, or if we alter the direction of their motion by causing them to strike the platform, then there will be less tension in the lower part of the chain than in the upper, as the tension in the lower part will be only that due to partially changing the direction of the motion of the links. The centrifugal force of the upper part of the chain will be therefore unbalanced, and will cause the chain to rise and keep its elevated position against the force of gravitation. If a quick upward motion is given to the platform, the chain may be thrown up in the air, and again dropped on the platform like a solid body. The next experiments are to show that centrifugal force may produce sufficient rigidity to cause a chain to run along a platform like a wheel. A short endless chain was put over a pulley which was driven at a great velocity; the chain was then dropped on the I platform, along which it ran for some distance. It is not necessary that the chains form circular loops to do this. The loop may be tall and narrow, and will, while running along, keep the longer axis of the curve in its original upright position. Nor need the chain be heavy. A watch-guard was hung over a pulley about eight inches diameter; it then formed a loop about eight inches broad by about two feet high. When thrown off the pulley it glided along the platform for some distance. The chains were also dropped on an inclined polished surface, on which they remained standing in rapid motion for some time. All these experiments only illustrate the balance of the centri- fugal force, and the tension when the motion is all in one plane. The next experiment is to illustrate this balance when the motion takes place in different planes. This is easily illustrated by means of a circular disc of paper, or any other flexible material. If we VOL. III. L 76 Proceedings of the Royal Society bend the disc while it is rotating, we find that the bent part does not rotate with the disc, and that the disc only slowly regains its original flat form. If we load the outside of the disc with a row of flattened pellets of shot, we increase the resistance or rigidity of the disc while in motion, and if the weight is such that it just balances the elasticity of the paper, then the bend will remain in the same place for a very long time while the disc is rotating rapidly. The disc may even be bent till the circumference touches the centre, and while the bend keeps its place the chain of shot is passing through many planes, and the tension at the different points just balances the centrifugal force. Before proceeding to experiment with the horizontal chain, I must refer to the disturbing forces in action causing the chain to change its form while in motion. When looking at these endless chains in motion, the most marked effect of this motion is to cause a curious reverse curve just after the chain has turned at the lowest point of its path and has begun to ascend. This reverse curve was supposed to be produced by friction from the great tension produced by the centrifugal force; but that it is not really so, is easily proved by taking two precisely similar chains and oiling one and passing the other through a flame to remove all grease. The only difference between the two chains now is that the friction in the one is greater than in the other. If we hang these two chains over two pulleys of the same diameter on the same shaft so as to drive both chains at the same velocity, we find that the oiled chain has the reverse curve well marked, while the friction in the other chain causes the loop to open out and take up a curve approaching a circle and shows no reverse curve, and when both chains are compelled to have the same curvature at bottom, the reverse curve is much the least where the friction is greatest. The reverse curve seems to be due to the change of motion which takes place in the links when moving in a path of varying curvature. For instance,, when the links are descending along the flat part of the curve, their motion is almost simply one of translation, whereas when passing round the curves they have a motion of rotation as well as a motion of transla- tion, the result of which is, that the links resist this rotation at the entrance of the curve, and thus flatten out the curve on that side, aud after the rotation has been communicated to them, they tend to 77 of Edinburgh, Session 1875-76. keep this rotation, and thus continue the curve at the lower end of the chain much farther round than if the chain was not in motion. And, for very evident reasons, the quickest part of the curve is not at the bottom, but a short distance up the ascending side; and farther, the rotation of the link at the bottom is quicker than that corresponding to the curvature. These points may all be illustrated by a chain in which the links are short and the chain as thick as possible, so that the moment of inertia of the links round an axis perpendicular to the plane of the motion of the links is as great as possible. Such a chain when properly made gives a series of large and well-marked waves all the way up the one side of the loop and down the other. The length of the links also tends to change the form of the curve. If we have two chains of the same material and same size every way, except in the length of the link, then the larger the link the more the chain tends to open out the curves and take the circular form, and the smaller the links the nearer it approaches the form it has while at rest, and the more marked the reverse curve becomes. An elastic band in rapid motion will also tend to take up a circular form, because the strain at the quick part of the curves will tend to open them out, in the same manner as when the band was at rest. An elastic chain while in motion does not show the reverse curve like a chain, probably because the strain on the material prevents it doing so. In the previous experiments gravitation acted on the chains, so that whatever form we might impress on them, gravitation con- stantly tended to change that form and bring it back nearly to the form it would have if gravitation alone acted on it. An attempt was therefore made to get quit of the disturbing effect of gravita- tion. Different ways were tried of effecting this, but none of them were thoroughly successful. The next experiment shows the most successful method tried, namely, suspension. The chain is hung by means of a number of fine cords to a circular disc, capable of rotating about a vertical axis placed as far above the chain as possible. The chain is driven by means of a rapidly revolving horizontal pulley running on a vertical axis, and to give sufficient friction the chain is pressed to the pulley by means of an elastic wheel. The centre of suspension is so arranged that it can be 78 Proceedings of the Royal Society brought over the driving pulley, or removed to some distance from it, so as to be able to bring the centre of suspension over the centre of gravity of the chain, whatever shape the chain may be caused to take. The chain so suspended, when in rapid motion, retains for a considerable time whatever form we please to give it. It may be moulded into a most complicated series of curves, and though it resists any effort made to alter these curves, it has itself but little tendency to do so. If we observe the chain closely, we will however find that the disturbing forces, which I have already referred to, are acting on the chain, tending to change its curvature. For instance, if we keep the point of suspension over the centre of gravity of the chain, we will find after some time that the chain will take up a circular form. This is caused by the friction in the chain, and other causes. Again, the effect of the varying rate of rotation of the link on its own axis is also well marked, but is quite different from what wo get when the chain is hung over the driving pulley. When the chain is hung over the pulley, there is a tension due to the wreight of the chain. This tension gives rise to the wave form which certain chains take up when in motion. The tension due to the centrifugal force has no such effect. When, therefore, the chain is suspended and gravita- tion removed, there is no tension preventing the chain from con- tinuing to curve always in the same direction; and if we use a chain specially prepared to show this effect, such as the one already referred to, the chain goes on bending further and further round till it comes against the part of the chain coming in the opposite direction and stops the motion, even though the chain at that point is also bending out of the way on account of the resistance offered by the links to rotation on their axis. of Edinburgh, Session 1875-76. 79 Monday, 3 d January 1876. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. On the Electrical Conductivity of Stretched Silver Wires. By J. G. MacGregor, M.A., B.Sc. Communicated by Professor Tait. The apparatus which I used in a few experiments on silver wires was as follows : — To a beam, supported in stonework, a plate of copper was fastened, upon which a smaller plate could be tightly screwed. Between the two plates a very thick copper wire was secured, vertically. Its lower end was provided with a small plate of copper, fastened by screws. This plate served to make fast one end of the silver wire under investigation. The other end was joined in the same way to a second thick copper wire; this was provided with a horizontal round brass plate, through the centre of which it passed, and which acted as weight-carrier. A length of about 8 mm. at the end of the part of the copper wire which projected below the weight-carrier was amalgamated, and, while hanging quite free, dipped into a glass cup containing mercury, which, by means of a long screw, could be elevated or depressed by any desired amount. When measurements of resistance were made it was always placed in such a position that the amalgamated part of the copper wire was just beneath the surface of the mercury. The glass cup served also to support the weight-carrier during the adjustment of the weights, that the silver wires might be sub- jected to no jerks. After putting on weights the cup was lowered very slowly and steadily until the weights hung free. A copper wire (4 7 mm. thick and 30 cm. long), dipping in the mercury, joined up the silver wire as one of the arms of a Wheatstone’s bridge. At the upper end of the copper wire, which was fastened to the beam, two other copper wires were fastened by binding screws. One of them went to the galvanometer; the other was the standard wire, with whose resistance that of the silver wires was 80 Proceedings of the Royal Society compared. For all the observations on a single wire, it had, in all cases, as nearly as possible the same temperature. That it might not be affected by warm or cold currents of air it was defended by a coating of gutta percha, and made to pass through a tube of water whose temperature could readily be noted. By dipping into a mercury pool it was joined up as a second arm of the Wheatstone’s bridge. A length of about 5 mm. of the end which dipped in the mercury was well amalgamated. Above that the wire was varnished by a non- conductor, so that contact began always at the same point of the wire. The other two arms of the bridge consisted of the segments of a Ger- man-silver wire, — Kirchhoff’s form of the Wheatstone bridge being used exactly as described by Wiedemann in his “Galvanismus.”* The galvanometer used was Wiedemanns mirror galvanometer, f the deflections of the mirror being observed by means of a telescope. The current employed was that of a Bunsen’s cell of great internal resistance. The length of the wire was determined by a very delicate cathetometer, which could measure accurately to *02 mm. The lower end of the copper wire which was fastened to the beam, was smooth and flat, and cut at right angles to its vertical axis. The edge of the small plate was correspondingly cut, so that the exact point at which the silver wire was seized and compressed by the copper plate could be seen through the telescope of the catheto- meter. The clamp which seized the lower end of the silver wire was arranged in the same way. The wires, of whose resistance measurements were made, were of pure silver, and were carefully drawn by M. E. Stohrer, philosophical instrument maker of Leipzig. They were always raised to a red heat before being subjected to tension, care being taken that fusion did not occur in any part. In order to determine the effect of tension on the conductivity of the wires, it was necessary to know the relation of their diameter before to their diameter after being stretched. This was estimated by a careful measurement of lengths and specific gravities. For the latter purpose a chemical balance was employed, which could weigh accu- rately to ’0001 grm. As the wires had to be rolled up to prevent their touching the sides of the vessel containing the distilled water in which they were weighed, the measured specific gravity was pro- * “ Galvanismus,” vol. i. pp. 251-255, 2d German ed., 1872. t “ Galvanismus,” voL ii. pt. 1, pp. 227-230, 2d Ger. ed., 1873. 81 of Edinburgh, Session 1875-76. bably not exactly that of the wire of measured resistance. The error, however, must have been very slight. The course of procedure was as follows : — The wire was heated red hot in an alcohol flame. After cooling, its specific gravity was determined. It was then fastened by the copper plates to the thick copper wires, and a slight weight was attached just sufficient to straighten the wire, that its length might be accurately ascer- tained (it was straightened as much as possible by being drawn between the fingers before being fastened in the apparatus). When straight enough for the determination of its length, its resistance was also measured by the method of double observation, as de- scribed in the u Galvanismus ” (see above).* After the determina- tion of resistance, weights were carefully piled upon the carrier, which during the operation was held fast from below. They were then allowed to stretch the wire gradually until it hung quite free, and its elongation had ceased. Then the length, the resistance, and finally the length a second time, were determined, the second measurement of length being made in order to be certain that there had been no further elongation. The weights were now carefully taken off, the carrier being again supported from below, and the specific gravity of the wire was measured as before, the compressed ends, however, having been cut off. A large number of experiments were rendered useless by the fact that too great weights were attached. Either the wires broke, or they were found on inspection to have too variable a diameter to be regarded as uniform. In the result given below such small weights were used that almost no difference of diameter throughout the whole length of the wire could be noticed by means of a magnifying instrument. Thus the wire could be treated as uniform, and the specific gravity method assumed to give its diameter. The results of the examination of three wires are given in the following table: — * Instead of the formula given in u Galvanismus,” the following was used: — s*+ - d2) + s(d1d12 + d%d12 - Zdxd^~ d^d^d^ — 0. The length of the German-silver wire as found by this formula was 1108795 mm. As measured by the cathetometer its length was 1108:8 mm. 82 Proceedings of the Royal Society Length (mm.) Weight (grms.) d* (mm.) Resistance (standard copper wire =unity). Length (length be- fore stretch- ing=unity). Resistance (resistance before stretching =unity). Wire 1. 1 777-62 809-56 2246 5075 198-8 239’8 1-4369 1-5519 1 1-0411 1 1-0800 Wire II. | 830-82 890-04 1246 6746 234-9 311-2 1-5376 1-7803 1 1-0713 1 1-1579 Wire III. | 660-86 729-14 1246 7911 114-7 216-9 1-2308 1-4864 1 1-1033 1 1-2105 These results agree, as might be expected, with those which Moussonf has published on steel, iron, and copper wires, in the fact that the resistance increases very much faster than the length. This must be the case unless there be a diminution of resistance, due to tension, sufficient to neutralise the increase of resistance due to decrease of the cross section of the wire. It is interesting to ask, then — Does the decrease in the diameter of the wire account for that part of the increase of its resistance which is not due to the increase of its length? The following table answers this ques- tion. The column headed “ calculated resistance ” contains the resistance as it ought to have been if its increase had been due only to change of dimensions; — Specific Gravity Observed resistance after stretching. Calculated resistance. Before stretching. After stretching. Wire I. 10-4784 10-5330 1-080 1-092 Wire II. 10-4967 10-5646 1-157 1*155 Wire III. 10-5051 10-5394 1-210 1-220 The agreement of the figures in the observed and calculated columns is very close, notwithstanding the many sources of error to which the experiments were liable, such as the change in * See Wiedemann’s “ Galvanismus,” vol. i. p. 255. t “Galvanismus,” vol. i. p. 310; “Neue Schweizerische Zeitschrift, ” vol. xiv. (1855), p. 33. 83 of Edinburgh, Session 1875-76. specific gravity produced by the rolling up of the wires, their extension by weight between the first determination of specific gravity and the first determination of resistance, the irregularity in their cross section produced by stretching, and the slight contrac- tion of the wires after the removal of the weights and before the second determination of specific gravity,— all of which, however, must have been exceedingly slight. It seems to warrant the state- ment that if tension has any effect upon silver wires at all the effect is exceedingly small. This differs from Mousson’s conclusion as to steel, iron, and copper wires. He found that the increase in their resistance produced by stretching was not fully accounted for by the change of their dimensions. In the course of the experiments I found that by raising a silver wire, which had been stretched, to a red heat, its resistance was very slightly diminished. A wire of about the dimensions of No. III., which, after having been stretched by 6985 grms. had a re- sistance of 1-8135, had, after being heated red hot, a resistance of 1-8103. This is again different from what Mousson has found to be true of steel, iron, and copper wires, but it agrees with a deter- mination made by Becquerel on silver wires.* The following tables contain series of observations made for the purpose of finding the relation between the stretching weight and the total increase in the resistance of the silver wires used. In these determinations, the constant resistance with which the resist- ances of the stretched wires were compared was that of a silver wire. Both wires were surrounded by a coating of steam. The stretched wire, in order that, by its being kept at a high tempera- ture, greater elongations might be produced by the same weights ; the constant wire in order that thermo-electric effects might be eliminated. The steam coating was formed by enclosing the wires in glass tubes, and these tubes in a much larger tube, and conduct- ing steam between them. In other respects the apparatus and mode of procedure were quite the same as before. The observa- tions were made when the appended weights had ceased to produce any appreciable elongation, and with the steam coating half-an- hour was generally found to be a sufficient length of time for the production of the total stretching effect. * “ Ann. de Chimie et de Physique” (3), xvii. 1846, p. 253. M VOL. IX. 84 Proceedings of the Royal Society able I. Weight (grms.) d mm. Resistance (Constant Silver Wire = unity). 500 102-0 •8315 750 99-8 •8348 1000 99-6 •8351 1250 98-8 *8363 1500 95-8 •8409 1750 91-4 •8477 2000 82-0 •8623 2250 63'0 •8925 Table II. 1285 60-6 •8963 1535 52-6 •9094 1785 426 •9260 2035 26‘6 •9531 2285 — *6 10011 2535 —42-2 1-0791 Table III. 873 4-2 •9924 1285 — 24-6 1-0453 1535 — 48-2 1 -0909 2035 —121-4 1-2459 Table IV. 1873 678-6 *2407 2873 676-8 •2419 3214 670-6 •2463* 4857 663-0 •2516 5171 659-6 •2540 5921 647-2 •2629 6490 635*0 •2717 6964 623-4 •2802 7650 600-8 •2971 8176 578-8 •3141 8307 567-0 •3233 8842 532-0 •3515 * This measurement is marked in my notes as “ inaccurate, owing to an error of observation.” 85 of Edinburgh , Session 187 5-7 6. It will be seen that the relation between appended weights and thereby increased resistances is not that of simple proportion. In this respect silver wires appear again to differ from copper wires. Some experiments made by Messrs Meik and Murray * having shown that the changes of resistance of copper wires, when stretched by weights, are directly proportional to the weights. I am deeply indebted to Professor Wiedemann of Leipzig, in whose laboratory these experiments were performed, for the excel- lent apparatus which he kindly placed at my disposal, and for the advice and assistance with which he favoured me. 2. On the Defoliation of the Coniferse. By Dr Stark. 3. On Diamagnetic Rotation. By George Forbes, Esq. M.A., F.R.A.S. Faraday’s discovery of the magnetic rotatory polarisation of light may be expressed in the following manner : — Let two electro- magnets, in the form of iron tubes, surrounded by helices of wire, be placed end to end, so that in the spaoe between them the lines of force are very intense. Let a rod of dense glass be placed in this space, so that a ray of light may pass through the two tubes and the rod of glass. Let such a ray on entrance be plane-polarised, so that the direction of vibration is in a vertical direction. If the electro-magnet be now magnetised, the emergent ray will be polarised, so that its vibrations are inclined to the vertical at a small angle. The direction in which the line of vibration has been rotated is the same as the direction of the positive current in the helices. The same effect might be produced without the aid of mag- netism if the rod were rotated round the axis of the ray of light with great velocity. The rotation of the plane of polarisation * Proc. Roy. Soc. Edin., Session 1869-70, p. 3. 86 Proceedings of the Royal Society would be the angle rotated whilst the light traverses the glass rod. This is on the assumption that the ether within the rod is likewise rotated. In the magnetic experiment it is easy to produce a rotation of 1° in a piece of glass three inches long. Light takes T.Tnrff, trmr, 777777 a seco,n6 to traverse this distance. Hence, to produce an effect equal to the magnetic effect, the glass rod would require to be rotated 10,000,000 times in a second. We cannot determine with great precision the plane of polarisation of a ray of light, hence we cannot measure any rotation of the plane of polari- sation which might be thus produced. In the same manner, if we suppose the molecules of glass and the accompanying ether to be rotated round the lines of magnetic force, and in the direction of the positive current producing the given magnetic field, then the phenomena observed by Faraday would be explained ; and we should be able to determine the number of rotations per second induced in any specimen of glass wiih a given intensity of magnetic field. So soon as the electro-magnet is demagnetised, the rotation of the molecules ceases. It seems, then, that there is a friction among the molecules tending to stop the rotation. Hence we should be led to conclude that the energy of the magnet is gradu- ally used up by the presence of the piece of glass. Assuming, then, that there is a friction among the molecules of glass, it follows that when the electro-magnet is magnetised the rod of glass has a tendency to turn bodily round an axis through its centre of gravity parallel to the lines of force ; and if the rod of glass were free it would turn round this axis. In the winters 1872-3 and 1873-4, I made a number of experiments to put this hypothesis to the test. The general idea of the experiments was this. A rod of glass was suspended by a fine skein of silk fibres between two poles of an electro-magnet, one pole above, the other below. A small mirror was fixed on the rod, and a lamp and scale arrangement was mounted for measuring rotations. Readings were taken when there was no current, and also in the two positions of the commutator. The result of these experiments seems to be that there is an effect of the kind anticipated. Sometimes, it is true, a deflection was produced by a diamagnetic repulsion, owing to a want of 87 of Edinburgh , Session 1875-76. absolute symmetry in the arrangements. This rotated the glass rod slightly, and produced a little confusion. But beyond this there was an undoubted effect, for the nature of the deflection was found to depend upon the polarity of the two poles, the effect being different according as the upper pole was a north or a south one. I was sometimes able, simply by timing the reversals of the com- mutator, to get up a very large rotation-swing, and by the same means I was able to stop the rotation swinging. I delayed the publication of these experiments with the view of establishing more certain results. But much time has elapsed, and I have still been unable to find time for this. Hence, I am unwilling any longer to withhold their publication. I will now give the experiments in detail, and will conclude by collecting the general results. Description of the Apparatus. A rod of glass was suspended by a strand of silk fibres attached to one end. This was supported on a stone imbedded in the wall of the laboratory. The rest of the apparatus was on a separate stand. A horse-shoe electro-magnet was placed so that the poles were vertically over each other, and as nearly above and below the axis of the glass rod as possible. Thus the axis of the glass rod lay along the lines of magnetic force. The electro-magnet was connected through a commutator with a battery of Grove cells. Upon the glass rod was attached a small piece of silvered glass, by means of which the light reflected from a paraffin lamp fell upon a scale divided to millimetres. The distance of the scale from the glass rod was about seven decimetres. The apparatus was arranged so that the glass rod was suspended within a glass jar or bottle, to get rid of currents of air. During the session 1872-73 thick flint glass tubes were employed for suspension, and an electro-magnet weighing about 6 lbs. After that a rod of Faraday’s heavy glass was used, and an electro-magnet weighing about 50 lbs. 88 Proceedings of the Boyal Society Details of Experiments. The first experiments were made in 1873, March 28, and they were continued regularly until April 16. The rod of flint- glass was suspended in air, water, and oil. A rotation was nearly always communicated to the rod when contact was made with the electro-magnet. When the magnetism of the electro-magnet was reversed I sometimes got a rotation in the opposite direction, and sometimes a rotation in the same direction, but to a different extent. The apparatus was repeatedly dismounted and set up again with all the parts changed. The effects were generally unaltered. In noting the experiments, I used the terms “no contact,” “right contact,” and “left contact,” as being least liable to lead to error. “ No contact ” means that the circuit was broken. “ Right contact ” means that the lower pole of the electro-magnet would, if free, point to the north. “ Left contact ” means that the lower pole of the magnet would, if free, point to the south. When the readings of the scale are increasing the glass is rotating in the direction of the hands of a watch with the face upwards. The glass was sometimes put into water or oil, and in this case also rotation was generally observed. The rotation oscillations in air were so great as to necessitate reading the scale at the end of each half oscillation, and taking a mean. In the following table each reading is a mean of many observations : — March 29. — Flint-Glass in Air. No contact, . 245 scale reading. Means. Right „ 155 L = 146, Left „ 146 R = 155. No „ . , 235 N = 240. Flint-Glass in Water. No contact, . 415 Right „ 268 L = 248. Left ,, 248 R - 268. No „ 410 N = 412. 89 of Edinburgh, Session 1875-76. Flint-Glass in Oil. Rio-ht and left contact each continued to diminish the scale o reading during twenty-two minutes. The change from left to right contact diminished the readings with a jump. “ No con- tact” again reversed the rotation. Flint-Glass in Water. No decided effect. No contact, Right „ Left ,, Flint-Glass in Air. 370 scale reading. 523 478 370 Means. N = 370. L = 478. R = 523. The poles of the electro-magnet were now put so far to the east of the glass as possible, and again as far to the west. The same kind of results were obtained. Oil was again used, and no certain effect was observed. March 31. — The apparatus, as left last day, with 'oil in the jar, showed no effect. No effect was shown with air. But on trying a new rod of flint-glass the old effects were observed. The oil seemed to have destroyed the effect. Flint-Glass in Air. Right contact, steady rise from 400 to 543 No contact, Left Right Left No Right No Left V 558 567 546 556 540 531 529 533 in about 4 minutes. R = 538. N = 542. L = 552. No contact, Right ,, Left „ Right „ Left ,, Half-an-hour interval. 522 x 512 523 497 519 508 ) R = 509. N - 515. L = 521. VOL. IX. N 90 Proceedings of the Royal Society By keeping right contact for decreasing rotation- swing, and left for increasing, the range of swing increased after 6 swings to 123 divisions. On reversing this action for 6 swings the range was reduced to 12 divisions. Note. — These are the most striking experiments. It will be noted that here the “ right ” gives lower readings than the “ left ” contact. But I cannot be sure that the commutator arrangements had not been changed. Here all disturbing effects are done away with, and the right and left contacts produce deflections on opposite sides of the “ No contact ” reading. No contact, Right „ Left „ No 5) Flint-Glass in Water. „ . 541 scale reading. Means. 531 R = 531. 551 N = 541. 540 L = 551. A new rod was now prepared, which also showed a very decided difference between right and left contact, right being lowest. Numerous experiments under various conditions were now tried, but no new effects were discovered. It is desirable, however, to record the following, which were made to be certain as to the direction of rotation under different conditions of polarity : — No contact, ....... 850 Upper pole would point to north if free, 840 No contact, ....... 848 Lower pole, 854 Upper pole, 835 Lower pole, 850 No contact, ....... 845 The general result of the experiments of the winter is, that when a 'pole tending to point to the north is above the glass rod , and a pole tending to point to the south is below , the rod turns in the opposite direction to the hands of a watch with the face upwards. On placing the magnet with the poles in a horizontal plane, rotations were sometimes observed. This is in direct contradiction to the theory that led to these experiments. I can offer no explanation, but merely record the fact. In the session 1873-74 similar experiments were made with a of Edinburgh, Session 1875-76. 91 piece of Faraday’s heavy glass. But in this case the glass was inserted in a hole in a cork, to which also the mirror was attached. On examining the cork it was found to be magnetic. This accounted for all the phenomena observed. But in the previous session this would not account for the phenomena. There was no cork employed ; and experiments made to test this by altering the position of the magnet showed that there was no magnetism in the arrangement. It was the doubt that hung over the last winter’s experiments that made me wish to delay publishing any results until I should have finally settled the matter. I have been unable to do so hitherto, and offer the original experiments in the meantime. Note on the preceding paper. [The first statement is that a rotation of the plane of polarised light might be produced by rotating a transparent body about the ray as an axis. It is improbable that no such effect would be produced, but that the question is by no means a simple one may be seen by looking at Sir W. Thomson’s paper on this subject (Proc. R. S. Bond., 1856). I have also tried a great many hypotheses besides those which I have published, and have been astonished at the way in which conditions likely to produce rotation are exactly neutralised by others not seen at first. There can be no doubt, however, that a rotation of some kind is going on in a diamagnetic medium under magnetic force, and this may be of the molecules of the glass of the ether or what not, and this probably goes on in all media whether transparent or not. This rotation, as Prof. G-eorge Forbes says, stops as soon as the magnetic force is removed. He supposes that it is stopped by friction, and therefore, that energy is being dissipated at all times as long as magnetic force acts on a medium. But we know that a magnet will retain its magnetism for a long time, and it has never been shown that a magnet must necessarily lose its magnetism. Hence we must admit that the molecular rotation is not accompanied with friction, but that it is set up by 92 Proceedings of the Royal Society electro-motive force, and exerts electro-motive force when it is stopped, like a rotating body having inertia. (a) If the friction supposed by Prof. Forbes exists, it would act as an accelerating force on the glass, so that if free it would rotate faster and faster up to a certain great velocity, and if suspended by a fibre, it would rotate till the moment of friction was balanced by the moment of tortion of the fibre. (J3) If there is no friction the only effects possible would be those due, not to the maintenance, but to the starting and stopping of the molecular rotation. To investigate (a) experimentally we must observe the elongations of the oscillation as follows : — Make + ve observe three turning points A. B C, break for nearly half a complete vibration. Make - ve observe three turning points D E F, break again, and make +ve, and so on. Then the result is obtained by taking I S { A + 2 B + C-(D + 2 E + F) } on when n represents the number of repetitions of the series of six observations. To investigate (J3) experimentally we must make and break when the mirror is passing the point of equilibrium. In Prof. Forbes’s experiments there is a disturbing effect due to the ordinary diamagnetic action of the electro-magnet on the tube, which, if the tube is not perfectly symmetrised about the axis of the fibre, will tend to produce rotation. This force, however, is the same whether the current be + or — , provided the position of the tube is the same. Hence, if the + and — currents are exactly equal, it may be possible to distinguish this effect from the effect sought by Prof. Forbes. J. Clerk Maxwell,] of Edinburgh, Session 1875-76. 93 4. On the Linear Differential Equation of the Second Order. By Professor Tait. ( A bstract. ) This paper contains the substance of investigations made for the most part many years ago, but recalled to me during last summer by a question started by Sir W. Thomson, connected with Laplace’s theory of the tides. A comparison is instituted between the results of various pro- cesses employed to reduce the general linear differential equation •of the second order to a non-linear equation of the first order. The relation between these equations seems to be most easily shown by the following obvious process, which I lit upon while seeking to integrate the reduced equation by finding how the arbitrary constant ought to be involved in its integral. Let u and v be any functions of x, du dv dx ^ dx A u + Bv u + Cv' u + Cv ■ ■ (i), where B and A, and therefore their ratio C, are arbitrary constants. The elimination of C from (1) must of course give a differential equation of the first order in £• We have _ u" + Cv" A/ + (V\2 * ~~ u + Cv \w + Cv/ Now we have, by adding and subtracting multiples of (1), &c., j., u + Pu + Qw + C(u -fPu+Qy) /u -\-Cvf ^ 1 Alf+cL/- * whence, if u and v are independent integrals of the equation 2/" + iy + Qz + mrj + 1 ^ (3), provided Q' p ^ + * 7W = m(^ i.e.. €-/Pdx ~jw - mf€ ' fFdx c lx , The next subject treated is the effect of the alteration of sign of P or Q in (2). This is illustrated by the equation y" ±xy' ±y = 0, which is integrable or at least reducible to quadratures for any of the four combinations of sign. The always integrable case where P = (C-a>)Q is next examined. Another portion of the investigation deals with certain infinite but convergent series, whose sums can always be expressed in terms of the integral of a linear differential equation of the second order. Consider, for instance, the expansion € X = + px +...•+■ 1+V X + + . . = 2 P nXn , suppose. Obviously we have Pn = p*P_n=^ + From this at once •)n+ 1 \n + P n + 2 |1 n + 1 j2 \n 4- 2 = Pn _ i , whence Pra = (/ dp)n P( dp • (5)- of Edinburgh, Session 1875-76. 95 Also d /Pn\ Pn + l | ^ 1 TV\Y)=Y+'' whence v'~* Yd dp\pn / p Eliminating Pw between (5) and (6), we obtain \dpj 0 \dpj Ip J (6). (7). This equation is thus true for all positive integral values of n, and its form at once shows that it is true for negative integral values also. It is very singular that such a series of equations of all orders should have a common solution. But it depends upon the fact, which I do not recollect having seen in print, that \dx ax/ \cLxJ \dxj This can be verified at once by applying it to xm\ as can also the companion formula ( d Y fd\* n [x — x) = x>h — ) xn . \ ax J \dx/ Suppose we had, instead of (5) and (6), f/Q/i d dq dq ( qnQn ) _ — Qn + 1 n— 1 Q» — ; (51), (61), we should find the same equation (7) for Q0 as for P0. In fact, as is easily seen, Q, = P». Other pairs which alike give the equation K, are and dr dSn ds = R n- f- 1 dr d / Pn\ _ R» — 1 \ rn J ~ rn — 1 (71) ’ dr d — Sre_i , ^s(sn Sw) — sn+1 Sn+i . We thus get the two distinct particular integrals of each of the corresponding differential equations. 96 Proceedings of the Royal Society More generally, and P n _ ( df Pn-i/ whence \dpj pn~v ’ P = (1_Y pn(±Y ” v \dpj “ \dpj pn~v Changing n - v to ra, this becomes — m p m m i which, when ra = 0, agrees with (7). Here n may have any posi- tive integral value not less than m. When we write n~m we have merely a truism. If we put n = m-f 1, we arrive at the same result as we should have obtained directly from the first forms of the equations (5) and (6). All these series satisfy differential equations of the form x cPy dx 2 = *• Corresponding properties are easily proved for the series forming the co-efficients of the various powers of x in the expansions of expressions like €^W + ^, €^ + ^\ &C, &C. It is easily seen that what has been called P0 above is the infinite series po= ^ + 12^32 + • • • = f(p) • • (8)> and that quite generally if n m _l+_P _j__£ I "I MiOm i pm 1 pm^pm &C. we have “-(4)V(4W'" n m whatever positive integer be represented by n. Of this the simplest case is U1 = €p > where of course of Edinburgh, Session 1875-76. 97 ni = ni • Again, just as the solution of this equation has the property cp _ cp + q € c — e , so it is easy to see that we have in (8) Ap) /(?) = ZO+2)i where the bracket over p + q is employed to indicate that in the expansion we must square the numerical co-efficients of each term of a power of this binomial, i.e ., P + q = p + q , p + q2- p2 + q2-\- 2 2pq , p -f- and express this by the help of an auxiliary operation in terms of a merely artificial quantity z, so that ^ + £2 = e*s Z ax so that all equations of the kind considered can he reduced to the very simple form C$ + i2 = kcax ax If this were integrated, the only remaining difficulty would lie in the separation of symbols from the quantities they operate upon. 5. On Two-dimensional Motion of mutually influencing Vortex- columns, and on Two-dimensional Approximately Circular Motion of a Liquid. By Sir W. Thomson. Monday , Yitk January 1876. The Bight Rev. Bishop COTTERILL, Vice-President, in the Chair. The following Communication was read : — On the Origin of Language— Max -Muller, Whitney. By Professor Blackie. Professor Blackie stated that though the origin of language might be considered by some more a metaphysical than a philological ques- tion, it was yet so closely connected with philology, that whatever opinions a philologer held on this question could not fail to exer- cise a strong secret influence on his philological procedure. The primary elements out of which language grew were admitted by all to be three, viz., cries or interjectional exclamation, mimetic re- production of audible sounds, technically but stupidly called onoma- topoeia, and gesture. But while agreeing on this threefold basis the most distinguished writers on this subject, such as Max-Miiller, Wedgwood, Whitney, Bleek, Schleicher, and Steinthal, disagreed fundamentally, or at least seemed to be at daggers drawing, with regard to the course which language pursued in its further develop- 99 of Edinburgh, Session 1875-76. ment. On the one hand, Muller, who had had a great influence in guiding public opinion in this region, stoutly asserted that out of the three primal elements, as from a root, no further growth of what we called human language, for reasonable social purposes, could take place; while, on the other hand, Wedgwood — who in this whole matter had, in his opinion, received scant recognition from the scholars of his own country — as stoutly maintained that from these three elements, as their natural root, the whole organism of the beautiful growth of language, stem, leaf, and fruit, could be satisfactorily explained. After carefully studying the arguments of the learned Oxford Professor, he was of opinion that Wedgwood was in the main right. To this conclusion he came from a course of independent investigation some years ago, and when, curiously enough, he had only used Wedgwood’s dictionary for occasional consultation, without having read and pondered the discourse prefixed to the last edition of that work. The grounds of his opposition to Muller were stated to be simply these : — While in perfect agree- ment with him that roots significant of ideas are the ultimate facts in the analysis of languages as we now have them, and believing also that such conceptional roots are the natural and necessary ex- pression of reason in a reasoning animal, and explicable only on the supposition of an indwelling plastic reason in man, I am at the same time unable to see why this plastic reason in the formative process of language-making should not have used the materials so amply supplied by the interjectional and mimetic elements of the simplest germs of speech. The interjectional element, I call the principle of significant vocal response ; and the onomatopoetic prin- ciple, I call the mimetic, dramatic, or pictorial element in language; and I am prepared to show that, even under the many defacements and obliterations which spoken words, like old sixpences or wave- worn pebbles, suffer from the tear and wear of time, they yet show in hundreds of cases on their face the manifest superscription of their mimetic origin. For we must take note, first, that not only pigs and cuckoos, cats, curs, and crows, but all nature, is full of sounds, and that there is no absolute silence anywhere but in death ; and, further, that not only an immense variety of sounds can be approximately expressed by imitation in articulated vocal breath, but that by an easy transference the impressions of the other senses can be analogically expressed in the flexible material of significant 100 Proceedings of the Royal Society sound. It is also not only an easy but a natural and necessary pro- cess of the human mind in the formation of general concepts to use the material presented by mere sensuous impressions ; and thus, while we expressly deny the perverse doctrine of the sensationists that mind can be explained from sense, or the imperial unity of thought be generated from a multiplicity of external impressions, we can see no difficulty in deriving such general concepts as char- acter and type , for instance, from the roots \apao-croi and TuVrco, which originally were mere mimetic reproductions of an external sound, as in our word scratch. Language, therefore, was formed by the gradual extension of words originally expressing sensations and feelings to intellectual purposes ; and there is nothing ignoble in this, for the mind uses the materials supplied by sense just as the architect uses the stones dug by the quarryman or the lime carried by the hodman. Neither can one at all see the logical justice of Max-Miiller when he exposes the historical falsehood of some of Wedgwood’s onomatopoetic etymologies; for the erroneous applica- tion of a principle does not in the least imply that the principle itself is erroneous; and, besides, the oldest roots to which certain very recent forms of Komanesque words may be traced back in Sanscrit can be shown in not a few cases to have been the product of that very mimetic process which Muller so persistently ignores. But while Muller seems actuated by some strange prejudice in his stout determination to make no use of the onomatopoetic element so thickly strewn in language, Professor Whitney has introduced no little confusion into this matter by talking of language as an insti- tution, and reviving the doctrine of the old Greek Sophists, that language is tfeVei, not cret. Every simile limps; but if we must have similes, it is far nearer the truth to talk of language as a growth and a living organism than to call it an institution. In some sense language is certainly a growth ; in no sense is it an in- stitution. Institutions like the Sabbath, for instance, are then creatures of positive law ; but language is a direct efflux of plastic reason, and no more an institution than the song of the nightingale or a sonata of Beethoven. As to the connection between Darwinism and the origin of language, while the Darwinian philologers, with Schleicher at their head, will no doubt find a special delight in tracing the splendid roll of a Platonic period from the grumph of 101 of Edinburgh, Sessio7i 1875-70. the primeval pig, and the mew of the pre-Adamitie kitten, those who with me look on Darwinism as a mere pleasant conceit of men besotted in the one-sided study of physical science, can, so far as philological conclusions are concerned, leave the conceit to shift for itself, being firmly convinced that whenever reason does show itself whether on the original appearance of man or at some after-stage of his development, it appears as a force altogether different from, and in some of its functions, as Professor Ferrier wisely maintained, essentially contradictory of, and antagonistic to, every kind and degree of mere sensation ; and in this character brings forth lan- guage as the natural manifestation and organised body of itself. Monday , 1th February 1876. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. Note on Certain Formulae in the Calculus of Operations. By Professor Stokes, Hon. F.R.S.E. (In a letter to Pro- fessor Tait.) “ January lith, 1876. “Formulae like those you sent me* are readily suggested by supposing the function operated on to be of the form %Axa, or say, for shortness, *«, with the understanding that no transformations are to be made which are not equally valid for 2Ar«. Thus fdL%dL\xa = a2(a— l)2 . . . (a — n -f Y)‘1xa~ n \dx ax) = a (a — 1) . . . (a — n + 1)^-^^ xu -(s)v(a)v‘ and (x x^ xa = (a+ l)(a + 2) . . . (a + n)xa + n = (a + ii)(a -j- n — 1) . . . (a+l) into which m and n enter symmetrically. Replacing the operations in the left hand member of the first formula by convertible operations, which will be separated by points, we find d d -i d d 7 J ^ X 7 • X i ) dx dx dx dx d d - 1 _2 2 d _i 2 d _i ~r x~r x — x 7-a; . x — x dx dx dx dx and so on. Hence, f f\n _ r~n( rn f r- n + ! dx x dx) \ dx x«-\ d x-n+2 V dx J Again, nLn- \ dx x X -n + 1 . n-lA «-n + 2 t *J 7 it/ dx = x — n n ( d Y ) 2 ( d\n n ( d\l Ms) » of Edinburgh, Session 1875-76. 103 2. A Further Contribution to the Placentation of the Cetacea ( Monodon Monoceros). By Professor Turner. In the year 1871, I read before this Society a memoir on the Gravid Uterus of Orca gladiator , in which I discussed the placenta- tion of the Cetacea. This memoir was published in the Transac- tions for that year. On the present occasion I purpose describing the placenta in a Cetacean genus in which it has not hitherto been examined. In the month of December 1875 I received, through the inter- mediation of my friend Mr C. W. Peach, from Mr John Maclauchlan, the chief Librarian and Curator to the Free Library, Dundee, a cask containing the gravid uterus of a Narwhal (. Monodon Monoceros ), which had been procured by the captain of the Dundee whaling steamer “Erik.” The uterus had been preserved in strong brine, and was in good condition for anatomical examination. The uterus was two-horned, and contained a foetus 5 feet 5 inches long in the left cornu. The gravid horn measured 7 feet 4 inches along its great curvature ; the non-gravid, 4 feet. The girth of the gravid horn, at its thickest part, was 4 feet 4 inches. The length of the corpus uteri was 1 foot ; that of the vagina, 1 foot 8 inches. The os was occluded by an extremely viscid mucus. The uterine cornua were opened into by a longitudinal incision along the greater curvatures. The uterine wall was comparatively thin, and the chorion was closely adherent to its mucous lining. By an incision through the chorion, along the greater curvature of the gravid horn, the sac of the amnion was opened into and the foetus exposed. The foetus lay with its back in relation to the greater curvature of the cornu, its belly to the lesser curvature, its head close to the corpus uteri; whilst its caudal end was directed to the narrow end of the horn, but did not reach to within two feet of the Fallopian tube. The tail was curved forwards under the hinder part of the ventral surface of the foetus. The pectoral flipper was directed backwards parallel to the long axis of the body. The umbilical cord was 3 feet long, spirally twisted, and bifurcating where it reached the sac of the allantois. The amnion formed an immense bag, which reached to 5 inches from the free end of the gravid horn of the chorion, but it did not extend into that part of 104 Proceedings of the Royal Society the chorion which occupied the non-gravid horn. The amnion was closely adherent to the greater part of the chorion in the gravid cornu ; but that portion of the chorion which was attached to the mucosa lining the lesser curvature of the cornu, and which lay opposite the abdominal aspect of the foetus, was in relation to the wall of the sac of the allantois. The allantois formed a large funnel-shaped bag at the place of bifurcation of the cord. It was prolonged along the concavity of the chorion to within 2 inches of its free end in the gravid horn, and to within 9 inches of the free end of the prolongation of the chorion into the non-gravid horn. The length of the sac of the allantois was therefore much greater than that of the amnion, though its capacity was much less. The allantois was prolonged as a slender tubular urachus into the umbilical cord, which also contained two large arteries and two veins. The amnion investing the cord had numerous brownish corpuscles, resembling those I have described in Orca gladiator , projecting from it ; and similar corpuscles were scattered over that part of the amnion which was in apposition with the wall of the sac of the allantois, and a few were seen on the amnion beyond the border of the allantois. In addition to these brown corpuscles, numerous other bodies of a dull white appearance were found. Sometimes these were slender rods, from j^th to j^-th inch long, arranged end to end like the links of a chain, at other times they were globular, like minute shot. The rods were most numerous on the abdominal half of the cord, whilst the globules were most numerous at and near its bifurcation. The surface of the amnion adjacent to the cord had a few of these globules scattered over it. These white bodies were covered by the smooth amnion, which with a little care could be stripped off as a distinct pellucid membrane. They consisted of crowds of squamous epithelial cells, so that in structure they resembled the whitish bodies which are so abundantly developed in connection with the amnion of the cow. Between 3 and 4 inches of the abdominal end of the cord was covered with cuticle, which had the purplish-grey colour of the cuticular investment of the adjacent surface of the wall of the belly. The two uterine cornua became continuous with each other through the corpus uteri, and were partially separated by an of Edinburgh, Session 1875-76. 105 imperfect septum, which projected from the inferior wall. Owing to the great distension of the left cornu, this septum was pushed to the right, so that the os uteri opened directly into only the gravid horn. The chorion extended from the end of the gravid to that of the non-gravid cornu. As it passed through the corpus uteri it was somewhat constricted by the projecting septum. In the whole length of the non-gravid horn, and at the free end of the gravid horn, the chorion was raised into strong longitudinal folds, which corresponded in reverse order with a similar series of folds of the uterine mucosa radiating from the orifices of the Fallopian tube. At the os uteri the mucosa was raised into strong folds, which radi- ated into the gravid chorion for a considerable distance, and in some parts of their extent projected as much as 3 inches from the general plane of the mucosa, though at the os they had not more than one half that projection. The chorion in apposition with this part of the mucosa was also folded. In the gravid horn opposite the foetus, where the expansion both ot chorion and uterus was the greatest, the folds were not present. Except in a few localities, to be immediately specified, the whole of the extensive surface of the chorion was so covered with vascular villi that, to the naked eye at least, no non-villous intervals could be recognised. The chorion was adherent to the uterine mucosa, so that gentle traction was needed to draw them asunder; and, as the one was peeled off the other, the villi of the chorion were seen to be drawn out of multitudes of crypts opening on the free surface of the mucosa. The chorion, which lay opposite the os uteri and the immediately surrounding mucous membrane, was for the most part not villous, but presented a smooth, feebly vascular appearance, which con- trasted strongly with the adjacent villous chorion. This smooth spot was irregular in form, measured 6 inches by 4 inches, and from it narrow bands of smooth chorion radiated outwards for from 2 to 3 inches between the villous covered folds of the chorion. It was similar to, but much larger, than the corresponding spot in Orca and the Mare. Small isolated patches of villi were scattered irregularly over the surface of this smooth spot. The inner surface of the chorion at the bare patch was lined by the amnion and not by the allantois. Three inches from this large spot a bare patch, 1 inch by inch, was completely surrounded by villous chorion, VOL. IX. P 106 Proceedings of the Royal Society The uterine mucosa opposite these smooth portions of the chorion was smooth and free from crypts, except where the isolated patches of villi were in apposition with it. Eadiating for about 1 inch from the pole of the chorion in the gravid horn were narrow non- villous bands of the chorion separated by intermediate villous surfaces. These hands corresponded to folds of the mucosa free from crypts, which radiated from the orifice of the Fallopian tube, and were continuous with the longitudinal folds of mucosa in that tube. In the non-gravid horn the chorion was devoid of villi for about 5 inches from its free end, and for even a greater distance the villi were irregularly scattered so that well-defined smooth patches could be traced as far as 10 or 12 inches from the pole. On some parts of the chorion pedunculated hydatid dilata- tions of the villi, about the size of small peas, were irregularly scattered. When examined microscopically, the villi were seen to be arranged in tufts, which varied in size and in the number of villi. Some tufts had not more than two or three villi, but more usually numbers were collected together, though occasionally short single villi arosefrom the chorion in the intervals between the tufts. The villi had as a rule a club-shaped form, but some divided into fili- form branches. They were highly vascular, and a beautiful extra- villous layer of capillaries was distibuted, as in Orca, beneath the free surface of the chorion. The free surface ofthe uterine mucosa had, as in Orca, a delicate reticulated appearance, and was pitted with multitudes of recesses and furrows, which again were subdivided into innumerable crypts. In the polar regions of the cornua and in the corpus uteri the mucosa was more spongy and succulent than in the greatly dis- tended part of the gravid horn, in which the mucosa was obviously more stretched, so that the pits and furrows were almost obliterated, and the crypts opened on the general plane of the mucosa. In their general arrangement, and in the vascularity of their walls, the crypts in the Narwhal resembled so closely the corresponding structures in Orca, that I need not give a special description. The layer of cells which lined them was a well-defined cylindrical epithelium, many of the cells of which, however, were so swollen that the breadth almost equalled the length. of Edinburgh , Session 1875-76. 107 Scattered over the surface of the mucosa in the more distended part of the cornu were numerous smooth, depressed, circular or ovoid spots, the largest of which was not more than ~th inch in diameter, though as a rule they were less than -j^th inch; so that to the naked eye they were apt to escape observation. Each spot was surrounded by a minute fold of the mucosa, sub-divided into crypts. On an average from twenty-five to thirty of these spots were found in each square inch. They resembled the smooth depressed spots de- scribed by myself* and some other anatomists in the uterine mucosa of the gravid pig. On the surface of the chorion adapted to this part of the mucosa, occasional smooth patches from -Ayth to-^th inch in diameter were seen surrounded by villous tufts which were in apposition with the smooth depressed spots on the mucosa, but they had not the definite stellate form which one sees on the chorion of the pig. The extra-villous layer of capillaries ramified beneath these non-villous spots of the chorion. In the succulent parts of the mucosa the smooth depressed spots could not be seen with the naked eye, but only after a careful search with a pocket lens were they found at the bottom of some of the trenches or pits in the membrane. From the general resemblance between these spots and those met with in the uterine mucosa of the pig, one was naturally inclined to think that they, would have a relation to the mouths of the utricular glands. I proceeded, therefore, to examine the glan- dular layer of the mucosa. The glands were very numerous, and branched repeatedly. Many of the branches formed short diver- ticula, others were much longer; sometimes they were tortuous, at others a considerable length of straight gland tube could be seen. In the deeper part of the mucosa the glands lay almost parallel to the surface; but as they approached the crypts, they were directed more obliquely, so as to be frequently divided in vertical sections. The glands were subjacent not only to the crypts, but to the smooth depressed spots, numerous examples of which I carefully examined. In one instance, I saw a tube lined by epithelium lying obliquely beneath the membrane of a spot, and opening near the middle by a distinct orifice bounded by a crescentic fold of the membrane. In * “Journal of Anatomy and Physiology,” Oct. 1875. Also Lectures on the Comparative Anatomy of the Placenta, Edinburgh, 1876. 108 Proceedings of the Iloyal Society a second instance, the end of a gland passed from under cover of the surrounding crypts, and then seemed to open by an obliquely directed mouth near the free edge of the spot. But upwards of thirty other spots examined with equal care gave me no evidence of gland mouths opening on them. Hence it would appear that these smooth surfaces on the mucosa are by no means necessarily associated with the mouths of the utricular glands, and one is disposed to conclude that the gland orifices are usually concealed amongst the crypt-like foldings of the mucosa. The very much greater number of the crypts than of the stems of the glands, negatives the idea of the crypts being merely dilatations of the mouths of the glands, so that in the Narwhal, as in Orca, the Pig, and Mare, the crypts are to be regarded as interglandular in position and produced by a hypertrophy and folding of the mucosa. Through the kindness of my friend Dr Allen Thomson, I have had the opportunity of examining a portion of the gravid uterus and chorion of a Narwhal, the foetus in which measured only 3J inches long. The free surface of the mucosa was gently undulating and traversed by shallow furrows, but no definite crypts could be seen. The gland-tubes were remarkably numerous, tortuous, and branching. I made a comparative measurement of their size, with that of the glands in my much more developed specimen, and found them to have only one-half the transverse diameter. The gland- stems inclined obliquely to the surface of the mucosa on which their orifices could occasionally be seen. The free surface of the chorion was not villous, but traversed by faint ridges, which without doubt fitted into the shallow furrows of the mucosa. Patches of epithelium-cells could be seen covering the surface of the chorion. It is clear therefore that in the Narwhal, as I have elsewhere de- scribed in the pig, the villi do not form on the surface of the chorion, nor the crypts on the surface of the mucosa, until the embryo has reached a stage of development in which its body, though small, has assumed a form which enables its ordinal characters to he recognised. When I published my memoir on the placentation of Orca, I was under the impression that the crypts were lined by a pavement epithelium, and was not disposed to regard the crypts in the mucosa of that cetacean as secreting organs; but a re-examination of Edinburgh , Session 1875-76. 109 of the epithelium-cells lining its crypts has convinced me, that they are not a pavement epithelium, in the sense of being squamous cells, but have an intermediate or transitional form between the columnar epithelium and the tesselated epithelium. In the Narwhal, again, the cells are cylindrical, as in so many mammals, so that I believe the Cetacea to offer no exception to the view that these cells are a secreting epithelium, and they doubtless elaborate a secretion for the nourishment of the foetus. From the fact that the utricular glands had a much greater calibre in my specimen than in the one belonging to Dr Thomson, one may infer that even after the crypts are fully developed the glands still play a part in foetal nutrition. The foetus in my specimen had an almost uniformly purplish-grey colour, but with a patch of yellowish-white on the belly near the anus. The snout was rounded; the fissure of the mouth 1J inch long; eye-slit inches behind the snout, and surrounded by a faint circle; ear orifice very minute, 3 inches behind the eye-slit; blow holes above and a little anterior to eye slit. Length of flipper 7 inches, its anterior edge 12 inches behind the snout. Funis was attached to the belly about midway between the anterior and posterior end of the foetus. A low, but distinct dorsal ridge, the rudiment of a dorsal fin, commenced a little in front of a point midway between tip of snout and end of tail, and ex- tended backwards for between 10 and 11 inches along the middle line of back. It had a lighter greyish tint than the surrounding skin. Breadth of tail was 15J inches. In a profile view of the foetus a slight depression in the contour of the top of the head was seen in the region of the blow-holes. The foetus in utero differed therefore very materially in colour from such a half-grown specimen as Dr Fleming described*, in wdiich the upper part of the body was a dusky black, the belly white, and numerous oblong- spots extended horizontally along the sides ; still more did it differ from old specimens, which have a whitish marbled colour. The presence of a dorsal ridge is also of interest, as the Narwhal is described as without a dorsal fin. I availed myself of the opportunity of examining the dentition of the foetus. On May 20th, 1872, I described to the Society the * Memoirs Wernerian Socy., 1811. 110 Proceedings of the Royal Society dentition of a foetal Narwhal 7J inches long, in which I found two dental papillae developed in the gum, on each side of the upper, jaw, but the early stage of development of the foetus did not permit me to say whether the anterior or posterior denticle would have been the one to become the maxillary tusk, though I thought it probable that the more anterior would become the tusk. In this much larger foetus the superior maxilla was 8| inches long. At the anterior end of each of these bones were two well marked sockets, one opening immediately behind the other. The anterior socket contained a cylindriform rudimentary tusk. The posterior socket contained an aborted tooth J inch long, and inch in its widest diameter. The hinder half of the aborted tooth was attenuated, and had several short irregular processes projecting from it ; the anterior half was smooth and rounded. This tooth was inclosed in a distinct sac, formed of fibrous tissue, which, like the sac of the rudimentary tusk, was firmly united to the fibrous tissue of the gum. There can be no doubt, therefore, that I was right in my conjecture that the more anterior dental papilla becomes the tusk of the Narwhal. 3. Observations on the Zodiacal Light. By C. Michie Smith. Communicated by Professor Tait. While engaged in cable work in the West Indies, I had, during the winter and early spring of 1875, a number of very favourable opportunities of examining the zodiacal light, Before leaving this country I had, under the advice of Professor Tait, and with a note of recommendation from Professor Jen kin, applied to the Royal Society for the loan of a spectroscope, to make observations with during the voyage ; but unfortunately I was unable to obtain one, and so had to content myself with a small pocket-spectroscope. On the outward voyage I did not notice the light at all till we got well to the south, near Cayenne, on the 8th of January ; and, owing to the very bad weather we had about that time, I was not able to make any satisfactory observations till we were again somewhat farther north. The general appearance of the zodiacal light has been so often described, more or less faith- fully, that I need not attempt any description of it here. I wish, Ill of Edinburgh , Session 1875-76. however, to mention one feature with which I was much struck, and which I have never seen remarked on — namely, that, on watching the western sky from sunset onwards, it is impossible to tell when the diffused sunlight ends and the zodiacal light begins till it becomes so dark that the form of the latter can be traced to a considerable altitude, when it is seen to be longer and narrower, and inclined to the vertical at a considerable angle. I am strongly inclined to believe that near the sun it is very much wider than at some distance from it, for I have very good reason to think that what by people generally would be taken as simply the last of the sunset glow is really due to the zodiacal light. This part, of course, can only be seen in places where the twilight is very short. The best time for making observations I found to be about two hours after sunset, when all traces of twilight had certainly dis- appeared, and consequently all risk of confusion with it was gone. On January 31st, in lat. 8°N., long. 56° W., the light was very bright, and I made some spectroscopic observations. At two hours after sunset the light was visible for 90° from the horizon, and so bright was it towards the horizon that I was able to get a distinct spectrum. I first opened the slit very wide, when I observed a broad strip of light, nebulous at the extremities, with a distinct reddish tinge at the one end ; then, by gradually closing the slit, I obtained a narrower but tolerably pure continuous spectrum, in which I could distinctly see reddish, orange, and greenish-blue, and on making comparison with the spectrum of a lamp (placed at the far end of the ship so as not to dazzle my eyes), I estimated that the spectrum extended from the red to past the position occupied by the F line in the solar spectrum. A large number of observa- tions taken on other nights, whenever the circumstances were favourable, entirely confirmed these first observations. On several nights, and especially on February 27th, when off Ponce, in the Island of Puerto Eico, I observed the spectrum from a short time after sunset till long after the last traces of twilight had dis- appeared, hut no change was noticeable after the spectrum had become so faint that the Fraunhofer lines could not be distin- guished, except in the brightness of the spectrum, as I was still able to see colour distinctly, but no traces of any bright lines. On February 26th and 27th I took a number of sextant measure- 112 Proceedings of the Royal Society ments of the zodiacal light. These are, of course, only approxi- mate, as the light has no definite boundary-lines, but gradually fades off at the borders. The measurements were made by the help of stars, as it was quite impossible to measure the light itself. On the 26th sunset was at about six o’clock, the light was very bright for 30° from the horizon, having at the horizon a breadth of about 25°, and at an altitude of 30° a breadth of about 20°. At 9 p.m. the light could be traced quite round to the eastern horizon, a phenomenon which I observed on several other occasions. At 10 p.m. the light was scarcely, if at all, visible. That this sudden disappearance was not caused by any change in the atmospheric conditions was clearly shown by the undiminished brightness of the stars. On February 27th the breadth at the horizon was 30°, while at an altitude of 30° it was only about 20°. The centre of the band passed a little to the south of the Pleiades. I endeavoured, by means of the sextant, to measure the inclination of the band to the vertical. For this purpose I chose two bright stars near the centre of the band — one at a considerable altitude, the other close to the horizon ; I then measured the angle between these and the angle between the upper one and the horizon ; these angles were respectively 55° 30' and 51°, giving the value of 31° 30' for the inclination of the centre of the band to the vertical. I had un- fortunately no access to star-charts, else I could have fixed the direction more accurately ; but even these rough observations con- firm the ordinary statement that the direction is slightly inclined to the ecliptic. The spectroscope used was one of Mr Ladd’s admirable small direct-vision spectroscopes, with five prisms and a single lens. Behind the slit is a small round hole, through which the light may be made to enter by opening the slit very wide, and which is very convenient for examining monochromatic light. With this in- strument it is easy to see a number of the Fraunhofer lines on a tolerably clear moonlight night. And such an instrument, though in some respects inferior to a simple large prism and slit, will, I believe, be found very suitable for work such as that described above, especially when it has to be carried on on board a ship much given to rolling. of Edinburgh, Session 1875-76. 113 4. Note on the Volcanoes of the Hawaiian Islands. By J. W. Nichol, F.RA.S. Communicated by Professor Tait. The late Transit of Venus Expedition gave the writer some opportunities of visiting several islands of the Hawaiian Archi- pelago, some details of which may prove interesting. They form a group of islands about 10J hours west longitude from Greenwich, and about 20° to 22° north of the equator, and differ in size from 10 miles long by 6 or 7 broad, to 90 miles by GO, which are about the dimensions of the most easterly and largest, viz., Hawaii (the Owyhee of Cook). The general lie of the islands is from north-west to south-east, those in the east displaying the most recent traces of volcanic activity. In the older or western portion the main mountain ranges run in the same direction as the islands, rising in many places to a height of 3000 to 4000 feet, and having lateral ridges branching off at right angles, with an occa- sional crater of oval shape thrown up at a distance from them, and evidently of more recent origin. The putting up of a meridian mark on one of these ridges in the island of Oahu was attended with some difficulty, the narrow space along which one had to ride, sometimes not more than a yard or two wide, with precipitous descents of 500 to 1000 feet on either side, not rendering it comfortable to any one with weak nerves. The two most easterly islands, viz., Maui and Hawaii, although having their greatest length in the north-east and south-west directions, are composed only of mountains standing singly, and present no appearance of ranges. Maui, indeed, is nothing more than a couple of mountains joined by a very low neck of land, on the top of the eastermost of which (Mount Haleakala), at a height of 11,000 feet, is found one of the largest and most perfect extinct craters in the world, being some 10 miles in diameter, which unfor- tunately time would not admit of our visiting. The sides of Haleakala are not precipitous, and the general view from the sea is that of a huge hog-backed mountain. Traces of flows of lava so recent as to be quite black, and not covered with vegetation, are also seen coming down from what had been openings in its sides a short distance above the sea-level. VOL. IX. Q 114 Proceedings of the Royal Society The island of Hawaii, or the most recent and easterly, is composed of four mountains — the Mauna Kea, 14,500; Mauna Loa, 13,800, Huallalei, 8000, and Kohala, about 5000 feet in height, with large valleys of 2000, 3000, to 6000 feet above the sea-level between. The slope of the mountains is usually gentle, and numerous small craters of 100 to 300 feet in height are found distributed on their sides, and also in the intermediate valleys. On the west side pre- cipitous rocks face the sea, with a height of 3000 feet, which have valleys opening seawards that are almost inaccessible from the land side, owing to the precipitous character of their sides. It is on this island that the most recent displays of volcanic activity are seen, the country having been overrun in many places by lava flows, which have left large tracks quite useless for agricultural purposes. Earthquakes are common, and the summit crater of Mauna Loa, 13,800 feet up, is frequently, and that of Killauea (on a level plateau on the side of Mauna Loa, about 3000 feet above the sea) is almost always in a state of activity. The crater of Killauea is on the north-east of Hawaii, about 32 miles from the bay of Hilo, which is the most convenient starting-point for those wishing to visit the volcano. In the ride of 32 miles one has an ascent of some 3000 feet, but the ups and downs are so numerous that one can hardly detect it. During some portion of the way one passes through very dense tropical vegetation, palms, tree ferns, &c., with creepers and ferns clustering around, but for the most part the path lies over lava flows, so recent as to be almost devoid of vegetation, which render it so rugged as to compel one to walk his horse the greater part of the way. When approaching the volcano the visitor is at first struck by the sight of hundreds of steam jets rushing up in all directions, some of which are utilised as vapour baths, by putting a wooden box over them with a hole in the top large enough to admit the neck of the bather. On going some hundred yards further, an immense pit appears, at the further end of which during the day are seen large volumes of smoke, while at night a red flare is visible in the sky, with an occasional piece of white hot lava getting tossed up high enough to be seen above the edge of the inner crater. This large pit or outer crater is of oval shape, and some 3 miles long by 1^ to mile broad in the widest part. The sides are precipitous, and from 600 to 700 115 of Edinburgh, Session 1875-76. feet in height, being in many places divided into close parallel ridges, showing the height to which the lava had reached before breaking out at a lower level. There were two large sulphur beds at the side of the outer crater, about 2 miles distant from each other, and pieces of native sulphur could be picked up, each with a hole in its centre, showing that the vapour had solidified round the hole from which it had emerged. The floor of the outer crater was composed of black lava, several acres of wdiich were covered over one night by the lava breaking out at a side of the lowermost edge of the outer crater, quite distant from the inner one. Our first descent was made at night by means of some rustic staircases cut in the sides of the ridges, and assisted by whatever brushwood might be growing on the sides. At last our party were landed on a floor of black lava, all seamed with cracks and contorted into curious shapes, sometimes like a mass of cable ropes mingled together, at others showing large pudding-like excrescences, which are dangerous to walk upon, since they are simply large bubbles with a thin covering, to guard against which each visitor carries a thick stick wherewith to test the ground before him. After walking for about half an hour on this black lava, and crossing innumerable cracks of from three inches to a foot in width, some of which showed a white line of fire about 6 feet beneath, the gradual ascent to the inner crater was reached. Its position in regard to the general form of the outer crater may be said to be in one of its foci, and its size, by estimation, about a ^ mile long by J broad. The increasing glare and smoke now warned us of our proximity to the more active parts, while here and there on the outer side of the inner crater were some bright red streaks, which, on our closer approach, turned out to be red hot lava flowing through holes in the outer side of the inner crater on to the general surface of the outer one. The ascent of some 70 feet to the top of the inner crater is a gradual one, and considerable detours bad to be taken to get round the parts which were being overflowed. The lava of its sides was twisted about and broken up in a most ugly manner, besides being so rotten as to break away in flakes whenever a foot was put upon it. The greatest caution was needed to test the ground before treading on it, and frequent play had to be made wdth our thick 116 Proceedings of the Royal Society sticks. Tumbles were frequent, from which the writer escaped unharmed by having a thick pair of dogskin gloves on his hands. One of our party, however, a professor from Indiana, managed to fall into a crack up to his middle, and got his hands severely cut and burnt. The view from the top, however, amply repaid the trouble. Four lakes of molten lava, the largest some 200 yards in length, and of kidney shape, and the others of smaller size, were seen in full activity. In the largest lake seven to eight fountains of white hot lava were playing up at once to a height of 30 to 40 feet, one sometimes stopping and another commencing at a different part of the side of the lake. The lava in this lake was about 50 feet below the inner edge of the crater, and appeared to be slowly advancing toward the tunnels from which we had seen it issuing on the road up. The lakes were not at the same level, and you might see one brimful and another 60 to 70 yaids off at a level of some 30 or 40 feet below it. On another of the lakes, about 50 yards wide, was a single fountain, bursting from a cavern in its side, and throwing lava half-way across its surface, while from the roof and sides of the cavern hung down lava stalactites. After looking at this for some time, the claims of our injured friend became so strong, as to oblige us to take him back to the crater house, resolved next da}^ to have a more deliberate inspec- tion. The next day proved wet, but the writer explored his way through the driving mist formed by the rain coming in contact with the heated lava, the only disagreeable incident being his getting to the leeward of a blow-hole, and having to run to get clear of the suffocating sulphur vapours. This blow-hole was about the size of a man’s body, and as you went forward to it you heard a gurgling sound beneath. Smoke was coming out in considerable volumes, and on looking in, the sides were seen to enlarge beneath and be at a white heat. Having at length got seated comfortably upon an upheaved block of lava about 20 feet above the larger lake, and 8 to 10 yards from its side, a new fountain sprung up suddenly from the side of the lake quite close at hand, which immediately forced a retreat to 117 of Edinburgh, Session 1875-76. a more respectful distance. About the same number of fountains continued to play up as on the preceding evening, and looked red by day. Daylight, however, drowned out the redness of the lakes as seen by night, and made them appear quite black. After watching for a considerable time, a red hot crack was seen to start suddenly from one side of the lake to the other, then other cracks in different directions, and first one-half of the lake and then the other was covered with a fresh coating of red hot lava, the former tumbling out of sight as it got shrunk and cracked in cooling. A curiosity called Pele's* hair is found round the sides of these lakes. This is composed of fine fibres of lava cooled, broken off from the molten liquid while being spouted up in the fountains, carried away by the wind, and lodged in the cracks around. The summit crater of Mauna Loa, some 15 miles off, and 10,000 feet above Killauea, was in activity about a month previous to our visit to the island, but limited time prevented our seeing it. Some points of curiosity may be noted before ending. 1. The lakes are not at the same level, although quite close to each other. 2. The summit crater of Mauna Loa is 10,000 feet above Killauea, and frequently in violent eruption, while Killauea is com- paratively undisturbed. 3. The outer crater of Killauea appeared to act as a receptacle for the lava, which, as soon as it arrived at a sufficient height, and got the assistance of an earthquake, broke through below and covered the country, sometimes running in a broad stream for 25 miles, and leaving an indication of the level which it had reached in form of a new ridge within the lip of the outer crater. 4. The necessity of an earthquake to enable it to break through is shown by the great difference of heights of the lava even within short distances. 5. The fountains were in every case playing round the edges of the lakes. 5. New General Formulae for the Transformation of Infinite Series into continued Fractions. By Thomas Muir, M. A. * The name of the Hawaiian Fire-Goddess. 118 Proceedings of the Royal Society 6. Laboratory Notes. By Professor Tait. (a) On a Possible Influence of Magnetism on the Absorption of Light, and some correlated subjects. Professor G. Forbes’ paper, read at a late meeting of the Society, and some remarks made upon it by Professor Clerk-Maxwell, have once more recalled to me an experiment which I tried for the first time rather more than twenty years ago, in Queen’s College, Belfast. I have since that time tried it again and again, whenever I suc- ceeded in getting improved diamagnetics, a more powerful field of magnetic force, or a more powerful spectroscope. Hitherto it has led to no result, but it cannot yet be said to have been fairly tried. I mention it now because I may thus possibly be enabled to get a medium thoroughly suitable for a proper trial. The idea is briefly this, — The explanation of Faraday’s rotation of the plane of polarization of light by a transparent diamagnetic requires, as shown by Thomson, molecular rotation of the lumini- ferous medium. The plane polarized ray is broken up, while in the medium, into its circularly-polarized components, one of which rotates with the ether so as to have its period accelerated, the other against it in a retarded period. Now, suppose the medium to ab- sorb one definite wave-length only, then — if the absorption is not interfered with by the magnetic action — the portion absorbed in one ray will be of a shorter, in the other of a longer, period than if there had been no magnetic force ; and thus, what was originally a single dark absorption line might become a double line, the com- ponents being less dark than the single one. Other allied forms of experiment connected with this subject were discussed. (6) On a Mechanism for Integrating the General Linear Differen- tial Equation of the Second Order. I am anxious to explain to the Society a kinematical device for the solution of the General Linear Differential Equation of the Second Order before I become acquainted with the principle of the integrating machine which, I understand, was described last Thurs- day by our President to the Boyal Society. 119 of Edinburgh, Session 1875-76. My arrangement consists of a combination of two equal modifica- tions of Ammsler’s Planimeter, ABC, AB'C', the wheels of which are attached at the joints B, B'. O' slides along AC, and the length of AC can be altered by turning either of the heads I), D', of coaxal screws of equal pitch. Now, if we suppose D connected with the wheel at B, and D' with that at B', by means of universal flexure joints (Thomson & Tait’s “ Natural Philosophy,” § 109), it is obvious that the length of AC will depend upon its angular position, and upon the motion of C' along AC. Let AB = AB' = a, BC = B'C'=6, AC = r, AC' = r15 / ABC = £, and let 0 denote the position of AC. Then, if the whole turn through an angle dO , the motion of B perpendicular to CB is the same as if it had rotated about 0, where [_ AOB is a right angle. Hence, if p be the radius of the wheel at B, dif/ the angle through which it rotates, ^2 ^ pd if/ = — a cos dO — ^ dO A similar expression holds, of course, for B'. Now, if a be the inclination of the threads of the screws, one right, the other left, handed, dr = p (dif/ — dif/f tan a , Now C' may be made to move along any curve we choose, so that r1 may be any assigned function of 0. Hence, by introducing the constant factor tan a ~w for r, we may give the equation the form dr dO r2 — © 120 Proceedings of the Royal Society to which the solution of the general linear differential equation of the second order can always be reduced. (c) The Electric Conductivity of Nickel. By C. Michie Smith and J. G-ordon MacGregor. Pure nickel foil, obtained in Paris by Dr Andrews, was cut into a spiral about 20 inches long, and it was on this spiral that all the following experiments were made. During the month of November 1875 a large number of experiments were made as to its thermo- electric properties, and these were found to be almost identical with that of the specimen from observations on which the line was laid down on the “ thermo-electric diagram.” (Trans. R.S.E., 1872-3.) This line, it will be remembered, is a peculiar one, and is very similar to that of iron, with this difference, that the peculiar changes take place at much lower temperatures in nickel than in iron. Having thus finally determined the position of the line in the thermo-electric diagram, we were anxious to discover whether, like iron, it exhibited other peculiarities about the same temperature, and for this end we made the following experiments on the electric conductivity at dif- ferent temperatures. The method of observation was as follows : — To the two ends of the nickel spiral stout copper wires were soldered, and the whole was carefully fastened together in such a way that no two coils of the spiral could touch each other. Side by side with this nickel spiral was placed a similar spiral of soft platinum wire of approximately equal resistance. This platinum was part of a wire the electric conductivity of which had been formerly carefully tested, and had been found to obey very strictly the law of being proportional to the absolute temperature. These spirals were then placed in a large pot of oil, care being taken that they hung quite free from the sides of the pot, and the ends of the thick copper wires were led to the pools of a mercury commutator, so arranged that either the nickel or platinum could be made to form one of the arms of a Wheatstone’s bridge, in connection with a very delicate Thomson’s dead-beat mirror galvanometer. In making the observations the oil was heated by a powerful Bunsen burner, and constantly stirred. By this means it was found per- fectly practicable to keep the oil sensibly at the same temperature during the time necessary to find the resistance of the two wires 121 of Edinburgh , Session 1875 76. by the ordinary balance method. That no errors were caused by thermo-electric effects was proved repeatedly during the experi- ments by completing the circuit without the galvanic cell, when no current was shown on the galvanometer. The results obtained for the nickel entirely agreed with what had been anticipated from the thermo-electric properties. For, when the conductivity is plotted in terms of the temperature, the curve shows a sudden change in direction at a temperature of about 149° C. (300° F.), indicating that there is at that point a sudden change in the rate of alteration of the conductivity with change of temperature. The curve ob- tained for nickel can be very well represented by two straight lines inclined to each other at an angle of about 9°, while the curve got for the platinum wire is strictly a straight line. That no part of the effect was due to the conductivity of the oil was amply proved by the following experiment : — Two pieces of platinum foil, each having a surface of 2*5 square inches, fastened to the ends of copper wires, were plunged in the oil when it was at a temperature of 550° F., and were kept a quarter of an inch apart; the resistance of the oil between them was then measured, and was found to exceed 9 megohms, while the resistance on causing them to touch fell to a small fraction of an ohm. After a series of experiments had been made with the nickel, the whole spiral was heated to a white heat in the flame of a Bun- sen burner, and allowed to cool in the air ; another series of ex- periments was then made on the conductivity, but no change was observed. The following tables contain the observations for two of the experiments, side by side with the values of the conductivity, calcu- lated on the supposition that the curves are best represented by straight lines — the platinum being represented by a single straight line, while the nickel is represented by a broken line. The calculated and observed values, it will be seen, agree very closely with each other, except where a divergence is to be ex- pected, namely, at the intersection of the two lines (nickel). The equations were taken from the lines obtained by plotting the con- ductivity in terms of the temperature. R is the resistance in thousandths of an ohm, t the temperature in degrees F. : — VOL. IX. R 122 Proceedings of the Boyal Society . January 14th, 1876. O o Nickel. Platinum, Formula up to t= 2729. R.='525 1 + 131. Formula R = -34 t + 176. 1 s-i Resistance = °^ms. Resistance =- ohms Ep 1000 1000’ Observed. | Calculated. Difference. Observed. Calculated. Difference. + — + — 53 159 159 • • • • • • 192 194 ... 2 69 168 167 1 200 199 1 ... 99 183 183 ... ... 210 210 ... • • • 132 200 200 • • • • • • 221 221 ... • • • 162 215 216 • • • 1 230 231 ... 1 194 233 233 • . . ... 242 242 ... • • • 218 247 245 2 ... 250 250 • • • • • • 247 265 261 4 • . • 260 260 ... • • . Formula above 1 = 272°. R = *775 t + 64. 279 285 280 5 ... 271 271 • • • ... 307 305 302 3 • • • 281 280 1 • • • 345 331 331 • • • • • • 293 293 ... • • • 376 354 355 • • • 1 303 304 • • • 1 440 401 405 ... 4 323 326 ... 3 January 18 th, 1876. Nickel. Platinum. O .4 P Formula up to t = 306°. R = '58 1 + 133. Formula R = '326 t + 187. Resistance = ohms -7- 1000. Observed. Calculated. Difference. Observed. Calculated. Difference. 102 194 192 + 2 • • • 219 220 + 1 136 212 212 • • • • • • 230 231 ... 1 169 230 231 • • . 1 242 242 • • • • • • 229 266 266 • • • • • • 262 262 • • • ... 301 312 308 4 ... 285 285 ... . . . Formula above t = 306°. R = -775 1 + 74. 363 356 355 1 ... 305 305 • • • • • • 407 386 389 • • • 3 319 320 • • • 1 447 420 420 • • • ... 333 333 ... • • • 502 466 463 3 • • • 348 351 ... 3 An attempt was made to discover whether or not the conductivity curve had another peculiar point corresponding to that in the 123 of Edinburgh, Session 1875-76. thermo-electric curve at a high temperature. For this an arrange- ment was used similar to that employed for the iron wire in the experiments formerly described (“ Proc. R. S. E.” 1874-75, pp. 629-631). But no results were obtained, owing to the breaking of the nickel ribbon when exposed to the great heat of the white hot cylinder. The following Gentlemen were elected Fellows of the Society: — William Skinner, Esq. J. Ballantyne Hannay, Esq. Peter Denny, Esq. Monday , 21 st February 1876. Sir WILLIAM THOMSON, President, in the Chair. The following communications were read : — 1. On the Structure of the Body-wall in the Spionidse. By W. C. MTntosh. In regard to external form, Nerine foliosa , Sars, is generally taken as the type of the family, and therefore it may be selected for structural examination in the first instance. Anteriorly the pointed snout is completed by the intricate interlacing of the muscular fibres beneath specially thickened cuticular and hypodermic layers. As soon as the body-wall assumes a rounded form, a layer of circular and oblique muscular fibres occurs beneath the hypoderm, the majority having the latter (i.e., the oblique) direction. In the centre of the area the oesophagus is suspended by strong muscular bundles (the most conspicuous of which are vertical) passing from the hypodermic basement-layer in the middle line superiorly to be attached to the oesophagal wall. A second series, as they descend to their insertion at the ventral surface, give lateral support to the tube; while a third group interlace in a complex manner, and, with the blood-vessels, fill up the space between the oesophagus and the wall of the body. Toward the posterior part of the head is found — on the dorsal surface — a slight hypodermic prominence, which indicates the position of the central ganglia of the nervous system ; the latter 124 Proceedings of the Royal Society being quite external to all the muscular layers, and covered only by the cuticle and hypoderm. In a line with the first bristles, the layers have assumed a more definite appearance. Beneath the hypoderm is a circular muscular coat, which, however, is somewhat irregular in its arrangement ; for, toward the dorsal region, the layer spreads out at each side, and the fibres mix with the oblique muscles of that part, while only a very thin layer stretches across the middle line of the dorsum. Within the former is a more or less developed longitudinal layer — best marked at the ventral aspect. A long oblique muscle extends from the lateral dorsal region on each side to the middle of the body-wall; and an important feature is the situation of the nerve-cord in close proximity to the inferior attachment of this muscle to the hypodermic basement-layer. Various muscular fasciculi, as before, attach the oesophagus to the body-wall, and the bristle-muscles and those of the lateral appendages have made their appearance. A little behind the foregoing it is noticed that the circular muscular layer is less continuous (though strong inferiorly), and that the longitudinal has been grouped by the other fibres into certain definite bands, the most conspicuous being a double dorsal and two lateral. The former fibres, indeed, have now assumed considerable bulk, a thin circular layer only intervening between them and the hypoderm. The formation of the lateral longitu- dinal muscles, again, is interesting on account of their homological bearings. From the inferior bristle-tuft, and from the region on each side of it, a strong series of muscular fibres converges toward the side of the oesophagus, and then splits into two bands. The outer bundle is the more powerful, and at the infero-lateral region of the body it bends somewhat sharply outward to be attached to the wall. The fibres thus arch over a chamber on each side for the lodgment of the ventral longitudinal muscle. In ordinary transverse sections they are much stronger than the other, and, moreover, have the nerve-cords at their insertion. The second series slants downward and inward, and is chiefly composed of fibres passing from the dorsal arch by the side of the oesophagus to mingle with the circular fibres at the ventral surface. A thin layer of longitudinal fibres also occurs on the internal aspect of the ventral transverse band (a part of the circular coat). of Edinburgh, Session 1875-76. 125 As we proceed backward, the lateral longitudinal muscles gradu- ally increase in breadth, while the great oblique bands nearly meet in the central line interiorly. The dorsal longitudinal fibres are grouped in two symmetrical masses, and a strong band passes between the edges of the ventral longitudinal muscles, — the median longitudinal fibres formerly indicated lying immediately within this layer. The nerve-cords have now descended quite to the ventral surface, and have a pale intermediate area. As soon as the body assumes a transversely-elongated form, the dorsal longitudinal muscles become much extended, and are, be- sides, intersected by the powerful vertical bands, which sweep from the dorsal basement-layer to the ventral surface, through the lateral longitudinal muscles (now for the most part ventral in position). The oblique muscle on each side is more horizontal, passing from the inferior bristle-bundle to the median line at the ventral surface, and going right through the vertical bands before insertion. The nerve-cords lie close together below the transverse muscle, and a small neural canal exists at the inner and upper border of each. There are still a few longitudinal fibres between the ventral attach- ments of the oblique muscles. The alimentary canal shows internal circular and external longitudinal fibres. It is very soon apparent, in proceeding backward, that the vertical muscles descending from the dorsal to the ventral surface do not interdigitate with the great longitudinal muscles through- out their whole extent. They leave, as observed by the lamented M. Claparede, at the external border of each dorsal muscle a con- siderable mass, which bends downward, and presents in transverse section a distinctly pennate appearance. A similar arrangement occurs at the outer and inner extremities of the ventral longitu- dinal muscles. Finally, the nerve-cords now have a single and very large intermediate neural canal. The foregoing condition continues with little modification to the tip of the tail ; though the dorsal pennate process disappears, the muscle itself being separated from its fellow, and considerably diminished in bulk, while the transverse fibres between it and the hypodemi have greatly in- creased.* * The late M. Claparede, in his “ Structure des Annel, S4dentaires,” p. 15, &c., pi. xv., gives the structure of the hypoderm, and notices the pennate 126 Proceedings of the Royal Society In Scolecolepis vulgaris , Johnst., the body-wall is similarly con- structed. Anteriorly the central ganglia of the nervous system lie outside the muscles on the dorsum, and the cords rapidly pass downward to the inferior attachments of the oblique muscles. In this region there is also a dense mass of longitudinal muscles. As soon as the oral aperture is completed posteriorly by the frilled hypoderm, the following arrangement occurs : — Within the hypo- derm is an irregular circular coat, the most conspicuous part being a broad belt, which hounds the mouth at the ventral border, and stretches between the great longitudinal muscular masses on each side. Superiorly a short but distinct band also appears under the central hypodermic elevation. A fasciculated longitudinal muscle (dorsal) lies below the latter on each side, its inferior surface being attached to a chitinous sinuous band, which forms a space by its upward curve from a raphe. A somewhat triangular interval occurs, moreover, between the muscles in the median line. The form of this chitinous arch is maintained by strong transverse fibres, which curve from raphe to raphe. At the latter, on each side, there is almost a rosette of muscular fibres, the chief fasciculi being directed downward and outward in transverse section. Out- side the foregoing dorsally are various oblique bands, the superior stretching from the dorsum downward and outward to the lateral hypoderm, while the lateral pass downward and inward. The chitinous arch gradually disappears as the dorsal muscle becomes fully developed. Behind the preceding region the arrangement consists, as in N.foliosa , of a double dorsal and two lateral longitu- dinal muscles, with the vertical and oblique bands, the latter passing through the former near the ventral attachment. There is also a very strong transverse ventral muscle, with a series of longitudinal fibres internally. Each nerve-cord in transverse section presents a distinct though small neural canal. The hypoderm, as well as the muscles, seems to be more largely developed than in N. foliosa , a feature corresponding with the increased size of the nerves. After the dorsal muscles have expanded into a broad layer, the same interlacing with the vertical bands occurs, but the pennate muscles and the arrangement of the nerve-cords of this form, but the fore- going observations do not interfere with his remarks. 127 of Edinburgh , Session 1875-76. arrangement formerly noticed does not appear in this form. The two neural canals soon increase in size, and approach each other in the middle line. With the exception of the great development of the ventral longitudinal muscles posteriorly, little further change takes place in the structure of the body-wall. The situation of the central ganglia in Scolecolejois cirrata, Sars., corresponds with the preceding, and the nerve-cords follow the progress of the oblique muscles toward the ventral surface, each trunk having a small neural canal. When the body wall is com- pletely formed (for instance about ^ in. from the snout), the great size of the longitudinal muscles is conspicuous. The dorsal form a thick superior arch, and proceed a considerable distance down the lateral wall; while the ventral muscles constitute two great curved masses in transverse section, the inner border of each being so carried upward that a deep ventral sulcus is formed for the nerve- trunks and their hypodermic external investment. For the same reason the strong oblique muscles are rendered nearly horizontal. The rounded firm nature of the alimentary canal gives little scope for the development of vertical fibres. The structure of the body-wall in Spio, and the position of the ganglia and nerve-trunks correspond with the foregoing in general features. The same may be said of the rarer Prionospio, which has two neural canals interiorly. In Polydora ciliata, Johnst., the body-wall anteriorly is charac- terised by the great development and bifid nature of the median ridge, which is flanked on each side by a prominent process of the hypoderm. In transverse section, the snout a little behind the tip presents, on each side of the dorsal process, a large rounded lobe, which projects downward to the oral aperture. Exter- nally, the lobe is composed of a thick layer of hypoderm, having internally a series of circular fibres, which come from the transverse dorsal arch in the form of a loop on each side. The fibres pass downward within the hypoderm, curve inward ventrally, and then proceed upward over the oesophagus to the point of commencement. A well-marked series of longitudinal fibres lines the outer division of the loop, and afterwards merges into the ventral longitudinal muscle of the side. The dorsal arch of transverse fibres cuts off the hypodermic process, containing the nerve-ganglia, and in the 128 Proceedings of the Royal Society cavity which forms therein is superiorly a small group of longitu- dinal fibres. Behind the foregoing a transverse dorsal layer is found beneath the central and now solid hypodermic process, next the dorsal lon- gitudinal muscles (the fasciculi of which, in the middle line, are directed downward and outward, while the outer are directed down- ward and inward); then a kind of X shaped process occurs in the centre, the legs of the X being prolonged horizontally, so that the whole resembles a figure of oo, the two spaces containing muscular fasciculi. The lateral and oblique muscles are largely developed, the latter having the nerve-cord on each side below its ventral attachment. The most interesting point in this form, perhaps, is the structure of the fifth body-segment, which bears the remarkable hooks characteristic of the genus, besides peculiar bristles with spear- shaped heads, and a minute fascicle of the ordinary structure. Immediately in front of the hooks, the body in transverse section shows externally a circular coat, which is thin at some parts, but greatly developed at others. Dorsally a very powerful series of fibres spread outward from the middle line on each side — some be- coming continuous with the circular coat, others passing obliquely outward and downward to the superior bristle-bundle. Inferiorly a strong transverse band lies over the nerve-trunks, and forms an external investment to the ventral longitudinal muscles. The oblique muscle comes from the lower bristle-bundle, and joins the former over the nerve-trunk, after piercing the vertical bands. The superior longitudinal muscle forms a great mass on each side, and it interdigitates with the fibres of the vertical muscle. The latter is greatly developed, especially at its inner border, next the oesophagus. The same (vertical) fibres pierce the ventral longitu- dinal muscle in the compartment formed for it by the circular and oblique bands. The size of the ventral is less than that of the dorsal longitudinal muscles. A somewhat strong group of longitu- dinal fibres lies within the ventral transverse band. Finally, each fascicle of the ordinary bristles has a V shaped series of fibres extending from the base of the tuft to the lateral wall, and inter- digitating with those from the transverse and other muscles of the region. 129 of Edinburgh, Session 1875-76. As soon as the powerful hooks of the fifth segment appear, the entire area — from the alimentary canal to the body wall — is occu- pied by their muscular apparatus. This consists of a dense series of fibres, which slant from the matrix of the bristles superiorly upward and outward to decussate with the fibres at the upper and outer angle of the body-wall. A still stronger series of fibres occur in the inferior division ; the inner are nearly vertical, the rest incline downward and outward. It would appear, therefore, that this powerful muscular mass chiefly acts on the hooks, so as to bring their curved points against the wall of the tube or tunnel. The strong inferior fibres likewise gain additional purchase by passing through the ventral longitudinal layer to be attached to the basement-tissue of the hypoderm. In this region the nerve- cords form two almond-shaped bodies in transverse section in the ventral hypoderm, and they are separated by a distinct interval. Posteriorly the nerve-cords still remain separate, and a large neural canal lies between them. A well-marked pennate process of the ventral longitudinal muscle occurs at its inner (median) edge. The foregoing forms, in conclusion, were compared with the structure of Mcea mirabilis , Johnst., an aberrant member of the Spionidas. 2. Note on Circular Crystals. By E. W. Dallas. At long intervals notices of circular crystals have appeared before this Society. In 1853 Sir David Brewster read a paper on the subject, which followed one by Mr Fox Talbot in 1836, and which again had been preceded by one from Sir David Brewster about twenty years before. It is not easy to account for these long intervals, unless they may be attributed to difficulty and uncertainty in manipulation, for except in very few instances the crystals observed by Sir David Brewster are of microscopic size, and, he remarks, require the perfection of optical appliances for their observation, and natu- rally so when crystals of the 200th of an inch in diameter are looked upon as of respectable size. Some time ago, being occupied with the subject, I found that by impeding crystallisation by means of gum arabic, circular crystals were formed of a greater size.* This took place with certain salts, * Perfect crystals were exhibited up to two inches in diameter. VOL. IX. s 130 Proceedings of the lioyal Society but not with all that were tried. Among the successful instances may be mentioned sulphate of copper, binacetate of lead, muriate of morphia, and other similar salts, which afford beautiful crystals, and are very easily manipulated. The method of proceeding is similar in all ; for instance, to a solution of sulphate of copper, let gum arabic or common dextrine be slowly added until it pours oily, then tried, and more gum or more salt added until the result is satisfactory. No precise general rule can be given, as each salt will be found different in the quantity of gum required. The solution is then to be spread thinly over a plate of glass, and dried rapidly before a clear fire, or, if the plate is small, it may be dried over a gas-burner. Upon cooling, the plate, if left to itself, soon shows numerous small specks, which will gradually develope them- selves into circular crystals. The process is hastened and a better result obtained by breathing on the plate, when, after a short time, they may be observed to start out very beautifully. These crystals while growing are extremely sensitive, any variation in the moisture applied for their formation resulting in the production of rings. The growth of the crystals once begun is extremely regular. When the centre is of inappreciable size they are circular, and they proceed onwards in that form until stopped by other crystals, or until the whole vacant space is oceupied by them. Should the origin have a definite shape, then that is carried on by the crystals arranging themselves always perpendicularly to the outline of that origin, while, should it be a straight line, they form beautiful fringes perpendicular to the line, and terminate at each extremity in semicircles. The centres round which the crystals arrange themselves maybe either some foreign body in the film, or be determined by some molecular arrangement of the salt at a particular point in the film. They seem to originate spontaneously, and subject to no apparent rule, for foreign particles, and even minute crystals, will not always determine centres ; in fact a film may be full of little crystals of the salt, and to very few of them can the circular arrangement be traced. The crystals present themselves under two aspects in all the salts that I have examined, — a true and an abnormal form. I designate the true form as that in which the crystallisation proceeds by the formation of spicular crystals radiating from a centre and 131 oj Edinburgh , Session 1875-76. in optical contact, while in the other many different forms may be observed, in which the component crystals are more or less of a laminate structure, often presenting most beautiful appearances. I have made this distinction, having observed that in some cases at least the true crystals are permanent, while the laminate are not so under like conditions, but change into the true form by time, or may become altogether disintegrated in a damp atmosphere into a confused mass, having few optical properties. The crystals also possess distinctive optical properties. The production of either of these classes of crystals appears to depend on two conditions, namely, on the thickness of the film, and on the amount of moisture applied in their production, — a thin film and a moderate supply of watery vapour inducing the true form, while a thick film and an increased quantity so alter the structure that at last, although the crystallisation may proceed from a centre, the circular character .is entirely lost. Spherical crystallisation, to which the circular is to be referred, is veryfrequent in mineral substances. It may be seen also in the well- known experiment of the rapid crystallisation of a supersaturated solution of acetate of soda, by the introduction of a centre round which the salt forms a spherical mass, and the surface, when the action has ended, presents all the appearance of a circular crystal. However difficult it may be to account for the origin of crystals, their growth in a circular form, when once the centre is determined in a film, is very obvious in those cases where they are produced. In the preparation of the film, not only is the superfluous solvent rapidly evaporated by heat, but a considerable part of the water of crystallisation is also driven off, and there is left on the glass plate a film of an amorphous substance, which, either by attracting moisture spontaneously from the atmosphere, or by having it added, allows the salt, whatever it may be, to resume its crystalline form. That this is the case may be seen from the fact that the crystallisa- tion will take place, and that in a circular form, if the drying of a plate is stopped just at that point when there is sufficient water left to enable the crystals to form when the plate is cooled. In this case their formation is a repetition of the acetate of soda ex- periment already alluded to. A plate may sometimes also be dried and crystallised, and on being again exposed to heat the crystals 132 Proceedings of the Royal Society will disappear, and the plate may be re-crystallised, but not so well as at first, and not from the same centres. This is the case with the binacetate of lead. There is one remarkable form of these crystals which is of fre- quent occurrence, and which Sir D. Brewster seems to have observed only in mannite. The form looks very extraordinary, a properly prepared plate presenting the appearance of being covered with paraboloids. These are simply circular crystals which have been formed in the film while the general crystallisation has proceeded from one side, and is caused by the crystals overtaking one another in their onward progress in one direction. Taking this case in its simplest form by supposing equal rates of crystallisation proceeding from the edge of a plate and from a centre near the edge, their line of contact will necessarily be a parabola, for it is evident the edge is a directrix and the centre the focus of such a figure, but this will very seldom occur, since the growths are not only generally unequal, but also vary in themselves. The question may be put whether gum arabic is the substance best suited for these experiments. I have not tried many, and with those that I have experimented upon the results were not so satisfactory. That other agents may be employed, according to the salts or other substances to be treated, is certain ; for example, collodion, as may be seen in a coated photographic plate that has been allowed to dry after excitation in the nitrate of silver bath, when circular crystals of iodo-nitrate of silver arQ often produced. This salt, be it observed, although produced through the agency of water, being at once decomposed by that element. Having confined my observations mainly to a very small number of salts, it would be premature to offer any general conclusion on the structure of their circular crystals or on their optical properties ; be- sides, from the great interest Professor Tait has shown in the subject, I am in great hopes that he maybe induced to make some investiga- tion in it. I shall only mention one point that I have observed in the effect of some crystals on the black cross, something in their structure producing a more or less spiral arrangement of the arms in a horizontal direction, while on one occasion a vertical arrange- ment was observed, in which the arms seemed to be raised one above the other like four quadrant steps. This effect I have only 133 of Edinburgh, Session 1875-76. seen once in a crystal of sulphate of magnesia, and have not been able to reproduce anything of the kind, hut the crystallisation of that salt is so varied and irregular that many things may pass unobserved. The only other point I shall lay before the Society is, that I have succeeded in producing a crystallisation very similar to that of frost- pictures on a window pane, and I hope to be able to make the imitation more perfect. For this purpose I have employed the sulphate of copper and magnesia, — a salt that crystallises under the rhombohedral system, the same with that of ice. This salt crystal- lises in the films from centres in a most remarkable manner in four different modes, viz., the true circular, the laminate, a branched or dendritic form, and another that I hardly know how to designate, unless it may he called the ostrich plume form. All these different forms may be observed on the plates, either simply or in combina- tion, and produce most varied and singularly beautiful effects. 3. Preliminary Note on the Flame produced by putting Common Salt into a fire. By C. M. Smith, Esq. (Com- municated by Professor Tail). PROCEEDINGS OF THE ROYAL SOCIETY OF EDINBURGH. vol. ix. 1875-76. No. 95. Ninety-Third Session. Monday , tith March 1876. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. The Annual Periods of Thunder (with Lightning), Light- ning (only), Hail, and Snow, at Oxford. By Mr Buchan. During the twenty-one years ending 1873, the maximum period of thunder with or without lightning, at Oxford, extended from about 9th April to the end of October, the middle of the period being the first week of July; the three highest days taken consecutively being those immediately preceding the summer solstice. During the five months from November to March, only thirteen cases had occurred during the period. Lightning, on the other hand, had its maximum period from May to November, — particularly during August, September, and October. The maxi- mum period of hail was during the first six months of the year ; whereas, during the second half of the year, very few cases occurred. The snow period extended from the middle of October to the middle of May, — most falling from December to March, — the absolutely highest month being March. Thus, thunder with lightning , at Oxford, closely follows the sun, the middle of the period being only about ten days after the VOL. IX. T 136 Proceedings of the Royal Society summer solstice; lightning (only) has its maximum period during that time of the year when the humidity of the air is at its maximum; hail is most frequent during that period of the year when the temperature is rising, or when the vertical layers of the atmosphere is in most unstable equilibrium ; and snow during the coldest months of the year, with this striking peculiarity, that the maximum period is not in the depth of winter, but in March, in the end of winter; immediately after which the curve abruptly falls. The intimate connection of the thunderstorm with summer rainfall, and the important bearing of the whole four curves on climatology, was referred to. 2. Note on the Origin of Thunderstorms. By Prof. Tait. This Note does not refer so much to those great thunderstorms which extend over hundreds of miles in each direction, as to those small local storms which are often seen of from two to five or six miles only in diameter. It refers particularly to those which are seen, in summer and autumn, to pass down the Tay valley. They almost invariably come from the westward, and I am told each is almost always accompanied by a storm of similar dimensions passing eastwards down the valley of the Forth. So far as I can ascertain, they seem both to commence almost abruptly somewhere in the district about Ben Ledi and Ben Lomond. Seen from St Andrews, which they frequently pass at a few miles distance to the northward, they usually appear to be in a state of rotation about a vertical axis. It is not very easy to judge of the relative distances of the various clouds, so as to ascertain the sense of the rotation ; but, in one case which I observed carefully last autumn, the rotation appeared to be in the positive direction, — i.e ., opposite to that of the hands of a watch whose face is turned upwards. If this be generally the case, and if it should be found that the direction of rotation of the companion storm in the Forth valley is negative , it would seem that their common origin may be explained on the following very simple hypothesis, which has the of Edinburgh, Session 1875-76. 137 additional recommendation of easily accounting for certain other singular phenomena. It is known from balloon ascents that, in general, the atmo- sphere is arranged in horizontal strata of considerable depth or thickness, alternately moist and dry, — temperature diminishing steadily with increase of height in the moist, and remaining nearly constant throughout the dry, strata. These strata have usually horizontal velocities, differing (sometimes considerably) both in magnitude and direction. Thus near the common bound- ary of two such strata, fluid friction will in general tend to produce vortex motion, — the vortex columns being at first nearly horizon- tal, with their ends at the boundary, which is a surface of discon- tinuity. A complete investigation of the possible circumstances would show four quite different cases : — Vortex formed into a stratum of dry ) moist j . f drj m ( moi ( moist 1 t dry 1 air. air. with its ends turning } down ) up J The half vortex-ring thus formed tends, so far as it can, to become semicircular. It may thus extend downwards to the earth or upwards into the higher regions of the atmosphere. If it extend downwards nearly to the earth, the lower portion will soon be destroyed by friction, and we shall have a couple of vertical vortex columns, with their ends respectively in the surface of dis- continuity, and on the ground. They will of course rotate in opposite directions about the vertical, and their mutual influence will tend to cause them to progress in directions parallel to one another, the motion of each being in the same direction as that of the rotatory motion of the side which it at the moment turns to the other. This is exactly the presumed case of the little storms in the Tay and Forth valleys above referred to ; the south side of the Tay column (that turned towards the Forth), moving eastward about the axis, while the axis itself moves to the east. This theory is evidently capable of at once explaining the ap- parently sudden occurrence of such storms (of which waterspouts must be looked upon as small but quickly rotating examples), when the lower atmosphere has for hours been in a dead calm. 138 Proceedings of the Royal Society The disturbance has, in fact, its origin above the lower stratum, and works its way downwards into it. It is also competent to explain the production of similar rotat- ing storms in the higher regions of the atmosphere — many miles above the earth’s surface — and thus to account for that by no means small number of cases of so-called “ summer-lightning,” which obviously cannot be explained by the occurrence of an ordi- nary thunderstorm at such a distance as to be below the specta- tor’s horizon. I have already explained to the Society that a possible source of at least a large part of the electric charge of a thunder-cloud is the contact-electricity of water-vapour and air. Thus while the precipitation of the vapour develops heat, the water particles pre- cipitated are strongly electrified. And the aggregation into one of a number of equal little drops all charged to the same potential may increase the potential in any ratio whatever. Thus the charge on each drop in a large cloud may become so great that the electricity is driven entirely to the particles at its surface. This is supplementary to, and does not interfere with, Sir W. Thomson’s explanation of the process by which the vapour is condensed. It is possible that taking place in greatly larger spaces of air, but to a much smaller extent in each cubic foot, this sudden pro- duction, and as sudden scattering in all directions, of considerable quantities of electricity, may account for some of the main pheno- mena of the Aurora. 3. An Application of Professor James Thomson’s Integrator to harmonic Analyses of Meteorological, Tidal, and other Phenomena, and to the Integration of Differential Equa- tions. By Sir W. Thomson. A first rough Model of Professor J. Thomson’s Integrator was shown. 4. Note on the Thermo-Electric Position of Cobalt. By Professor Tait, 139 of Edinburgh, Session 1875-76. 5. On a Glass Digester in which to Heat Substances under Pressure. By Dr E. A. Letts. The objections to the use of sealed tubes are known to every practical chemist, and are a serious drawback to their employ- ment. The chief of these are the time expended in the manu- facture of the tubes, the amount of skill in glass-blowing re- quired, the danger experienced in opening them, and above all, the fact that only a small quantity of material can be heated at one operation. Moreover, the same tube can seldom be used for more than three or four experiments, as each time it is sealed up its neck must be drawn out, and its length thus considerably decreased. These disadvantages were especially felt by me whilst preparing bromacetic acid, which was required in considerable quantities, and where as many as half a dozen tubes of bromine and acetic acid had to be heated before 100 grammes of the acid could be obtained. To obviate these objections I have had an apparatus constructed, which consists of a cylinder of glass, the walls of which are about half an inch thick. Its length is fifteen inches, its external diameter three inches, and its capacity about 600 cubic centimetres. At one end it is drawn out to a tube, whose aperture is only about one-sixth of an inch in diameter, though its walls are as thick as the rest of the apparatus. Origin- ally this tube was provided with a stopcock, but at Professor Brown’s suggestion, I have substituted a glass plate, which is ground fiat, and accurately adapted to the top of the tube. In order to keep the glass plate pressing on the tube the whole apparatus is placed in a frame, consisting of three brass wires arranged symmetrically around the cylinder, and attached by means of nuts, below, to a brass ring, and above, to a brass plate, through which latter a screw passes, which, when turned, presses on a brass plate placed on the glass cap. As any experiments with such an apparatus would be attended 140 Proceedings of the Royal Society with danger, were it necessary to be in its neighbourhood, it occurred to me that an automatic arrangement might be employed to give notice that the temperature had been reached to which it was intended to subject the digester. For this purpose I employed a thermometer with a somewhat wide tube and large bulb. A platinum wire is sealed into the bulb, and touches the mercury, whilst a brass wire passes down the tube, and is held in position by a binding screw. The two wires are connected with an electric bell, the brass wire being so adjusted, that when a particular temperature is reached the mer- cury touches its end, and thus completes the circuit, and causes the bell to ring. In order to test the digester, about 200 grammes of a mix- ture of two-parts bromine and three of acetic acid was placed in it, and after fixing it in its frame, the whole apparatus was immersed in an oil bath and heated to 150° C., the temperature at which reaction in this case takes place. The experiment was made in a cellar, and the bell placed in a room some distance off. The gas to heat the oil bath was led by a tube from another cellar, so that it could be regulated without going near the digester. In about an hour and a half the bell rung, and thereupon the gas was shut off; and on examining the digester next day, it was found that the reaction had taken place, and that only twelve grammes of product had been lost — a very inconsiderable quantity. As the action of bromine on acetic acid is very sudden, and accompanied by the disengagement of a large volume of hydro- bromic acid, the apparatus may be considered to have undergone a very severe test, and that its efficacy for all ordinary purposes is established. Should the digester come into general use, it will certainly save chemists much time and labour. The following Gentlemen were elected Fellows of the Society : — Rev. Francis Le Grix White, M.A. James Duncan, Esq., Benmore. Rev. Norman Macleod. J. S. Fleming, Esq. James Douglas H. Dickson, M.A. Glasg., B.A. Camh. of Edinburgh, Session 1875-76. 141 Monday , 20 th March 1876. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. On the Connection between Cohesion, Elasticity, Dilatation, and Temperature. By Professor George Forbes. (. Abstract .) At various times there have arisen supporters of one or other of two extreme hypothesis concerning the nature of what we define as force. These are the hypothesis of u action at a distance” and of “ no action at a distance.” According to the latter hypothesis, the centre of gravity of no body, however large or however small, can be moved from a posi- tion of rest, nor can its motion be altered in direction or amount, except by direct collision with another portion of matter. Starting from this supposition as a basis of argument, and without assuming anything further as to the manner in which the different physical forces are caused by collisions, it is possible to arrive at some very general theorems; and from these theorems conclusions may be drawn as the nature and connection of some of the physical forces, which are necessarily true if the hypothesis of no action at a distance be true. The principal result of these theorems is the following: — Let a rod be chosen of any substance whose cohesion and elasticity do not vary enormously with the temperature. Let a be its expan- sion, in terms of its length, when the temperature is raised 1°. Let /3 be the compression of the same rod, in terms of its length, when a unit weight is supported at its summit. Let c be the number of these units which, when suspended by the rod, suffice to break it by sudden rupture. Let 0 be the absolute temperature at which all these experiments are made. Then the theory leads us to the conclusion that Only a few experiments have been made by which we can test 142 Proceedings of the Royal Society this law. But the following values are the most accurate, and tend to prove the truth of the law. The apparent discordance in the case of iron is in part due to the variations in the qualities of that metal in different specimens. /8c e a Gold, •00001484 •00001358 Silver, .... •00001796 •00001809 Copper, .... •00001511 •00001481 Platinum, . . . •00001006 •00000851 Iron, •00001573 •00001220 In calculating this table, the values of c from the experiments of M. Wersheim are used; those of a from the experiments of Mr Mathiessen (except iron); those of ft from the experiments quoted by Prof. Balfour Stewart in his Text-Book; and the assumed temperature is 18° C., or 283° absolute temperature. 2. Notice of the Completion of the Works designed by Sir Charles A. Hartley, F.R.S.E., for the Improvement of the Danube. By David Stevenson, Esq., V.P.R.S.E. In 1868 I presented to the Society, on behalf of Sir Charles A. Hartley, a memoir published by the European Commission of the Danube, on the improvement of that river, and at the same time gave a notice of the works designed by Sir Charles Hartley for effecting that important object. These works have now been com- pleted, and Sir Charles Hartley has again asked me to present to the Society a second memoir published by the Commission, which brings the history of the works constructed under their charge down to the time of their completion in 1873. In supplement of the notice formerly communicated, which referred to a work in progress, it may not be uninteresting, now that the work is completed, to state briefly what has been effected by this most important and successful example of hydraulic engineering. of Edinburgh , Sessio7i 1875-76. 143 The engineering problem to be solved by the European Com- mission was the removal of the bar which obstructed the Sulina mouth of the Danube, which, in 1856, had a varying depth of channel never exceeding 11 feet. The design of Sir Charles Hartley — the engineer to the Commission — consisted in piers so constructed as to confine the current of the river in its passage into the Black Sea. At the date of my last notice the north pier had been extended to the length of 4640 feet, and the south pier to 3000 feet, and a maximum depth of 17J feet instead of 11 feet had been obtained. I, however, suggested in that notice, that as the Danube must continue to bring down an enormous mass of detritus, so in course of time the works which had proved so successful must be extended; and it appears that this has been found necessary, as the south breakwater, completed in 1871, has been extended to 3457 feet in length, and even with this additional length it is, I think, not improbable that in the course of time still farther extension may be required, for the Sulina mouth of the Danube will still dis- charge the same amount of water, bearing with it the same amount of alluvial matter, estimated in high floods at about 70,000 tons in twenty-four hours, the deposit of which at the extremity of the piers will still have a tendency, though in deeper water, to form a bar. The works have, however, proved most successful, and reflect the highest credit on Sir Charles Hartley, by whom they were designed and executed, and the following is a summary of the results that have been obtained. The total length of piers executed is 8789 feet, at a cost of L. 185, 352, being L.21 per lineal foot, in an average depth of 14 feet at low water. The navigable depth of the channel over the bar has been increased from 11 feet in 1856, to 20 feet in 1873. In 1853,2490 vessels, of 339,457 aggregate tonnage, left the port; in 1869 there were 2881 vessels, with a tonnage of 676,960. Thus, while the number of vessels increased only at the rate of 16 per cent., the tonnage, due to the greater draught, had been increased at the rate of 50 per cent., a good practical proof of the value of the improvements. The number of shipwrecks at the mouth of the Danube has also been greatly diminished. VOL. IX. u 144 Proceedings of the Royal Society Monday , 3 d April 1876. Sir WILLIAM THOMSON, President, in the Chair. The following Communications were read : — 1. Chapters on the Mineralogy of Scotland. By Professor Heddle. Chapter I. —On the Bhombohedral Carbonates. Communicated by Professor Tait. Professor Heddle read a paper on the 11 Bhombohedral Carbonates occurring in Scotland,” the first of a series of Chapters intended to embrace the analytical results of an investigation of all unknown or insufficiently determined Scottish species. In this paper many analyses of the carbonates were submitted ; and the pseudomorphic changes taking place in these were referred to in a special manner. 2. On Thermo-Dynamic Motivity, By Sir W. Thomson. 3. On the Vortex Theory of Gases, of the Condensation of Gases on Solids, and of the Continuity between the Gaseous and Liquid State of Matter. By Sir W. Thomson. 4. On two new Laboratory Apparatus. By William Dittmar. The object of this communication is to submit to the notice of the Society two little inventions of mine, which, whatever may be the degree of originality which they can claim, will, I venture to hope, prove useful additions to the catalogue of chemical-laboratory appliances. The one is a new form of the precision balance, which pretends to execute exact weighings with a hitherto un- attained degree of rapidity ; the other is a contrivance for main- taining a constant pressure in a supply of gas, and thus making it possible, with comparative facility, to keep, say an air-bath, for any length of time, at a constant temperature. The new balance differs from the instrument in its customary 145 of Edinburgh , Session 1875-76. form only in two points, of which the more important is a modifi- cation of the centre of gravity “ bob” arrangement, which enables one, at a moment’s notice, to shift the centre of gravity of the instrument from a certain definite position, I., to .a certain other (higher) position, II., matters being arranged so that in passing from I. to II., the sensibility, i.e. the deviation, correspond- ing to an overweight of, say 1 milligramme, is increased in an exactly pre-determined ratio, such as of 1 : 10, for instance. For this purpose the “bob” is made very light, so that the distance through which it has to travel in order to effect the desired change of sensibility is not too small, and, instead of to a screw as usual, is fixed by mere friction to a vertical triangular steel rod forming part of the needle. The other new feature in the balance is, that the rider-principle, besides being discounted in a slightly different manner from the customary one, is extended to the determination of differences of weight up to 100 (instead of 10) milligrammes. The arrangement adopted is represented in the accompanying sketch, for the interpretation of which it is only necessary to say that C (10) and (10) O are equal to C (0)x and (0)1 (10)j respectively, and that both O (10) and (10)j are each divided into 10 equal parts, the former by notches filed into the beam, the latter by marks ; and to add, that there are two riders, one weighing^ centi- grammes for the left arm, and another weighing p milligrammes 146 Proceedings of the Royal Society for the right arm, the balance being adjusted so that, when both riders are at their zero-points, it is in equilibrium, and p being chosen so, that, supposing the large rider to be shifted to the n mark, and the small one to the m mark, this virtually amounts to the addition of lOn + ra milligrammes to the charge in the right pan. There is no need of my explaining how the balance is meant to be used; I will rather avail myself of this opportunity for drawipg the attention of readers interested in the subject to a few inferences from the theory of the balance, which, obvious as they are, have hitherto not been sufficiently appreciated by either the authors of our physical handbooks or by practical balance-makers. I. Given a balance in which everything is constant except the distance s of the centre of gravity of the empty instrument from the axis of rotation, and it is easily shown that (for a constant charge) the deviation a of the needle for a given over-weight A, and consequently the “sensibility” a — is the greater the less s. This, of course, is duly stated by all authors; but what is always forgotten to be pointed out are two things, viz. — 1st, That the “ sensibility ” has nothing to do with the inherent precision of the instrument ; and 2dly, That supposing the sensibility to be increased, all the other good qualities of the balance get less ; we diminish the rate of vibration (this rate being proportional to we diminish the range of differences of weight deter- minable by the method of vibration ; we diminish the relative constancy (in opposition to variations in the charge) of the sensibility and the time of vibration. Considering now, — II. The case of a balance to be constructed , the arm-length l and weight w of the empty beam also become variables, related to each other, according to some equation like w = const. l7 and (assuming each of the pans to bear a certain medium charge p) we have t i— - — t== const. J l v const. + const. I , sja i.e ., by diminishing l we can increase the sensibility without diminishing the rate of vibration (or vice versa)) but the other 147 of Edinburgh , Session 1875-76. disadvantages mentioned under I. must be taken into the bargain, and, besides, the inherent precision of the balance gets less.* To pass to an example: What we gain by substituting a 7-inch for a 14 inch bea,m is that, for the most convenient t, the sensibility becomes 2 to 4 times greater; but this advantage is secured with- out expense in good qualities by placing before the graduated limb a lens magnifying the excursions of the needle into 2 to 4 times their natural size. This is the theory of the u short beams” which have lately come so much into fashion. To come back to my own balance, I must not forget to thank Messrs Becker Sons of Rotterdam for the readiness with which they have, at their own risk, tried to realise my ideas in an actual instrument, which, by the way, is now being exhibited at South Kensington. To increase the usefulness of the instrument, I have caused Messrs Becker to add to it a glass plunger, which is adjusted so that it displaces exactly 10 grammes of water at 15°, and which consequently enables one with great rapidity to determine the specific gravities of liquids by tbe method of immersion. To pass now to the new gas- governor , its most essential part consists of a mercury-manometer (fig. 2), of which one limb. A, is about 20 mms. wide, and stands vertical ; while the other, C, is of the width of a thermometer tube, and is placed horizontally. * For fuller explanations, see my article “ Balance ” in the “ Encyclopaedia Britannica.” 148 Proceedings of the Royal Society The empty part of the wider limb communicates, through F, with the gas-supply, through G- with the gas-lamp serving to heat the air-bath; and the quantity of mercury is adjusted so that, when the gas is at the lowest pressure which, in the course of the experiment, it is likely to “assume, the mercurial index in C occupies a certain convenient position a. The manometer is connected with a constant battery (the circuit of which includes an electro-magnetic arrangement for opening or shutting the gas-tap), in such a manner that, as soon as, through ah increase of pressure in E, the index in C travels ever so little towards the right of a, the current is closed, and the gas cut off. The following Gentlemen were elected Fellows of the Society : — John Macmillan, M.A. John Gibson Cazenove, D.D. The following Gentlemen were elected Honorary Fellows of the Society : — 1. Foreign Honorary. Carl Ludwig, Leipzig. Ferdinand de Lesseps, Paris. 2. British Honorary. Henry John Stephen Smith, Oxford. Thomas Henry Huxley, London. Thomas Romney Robinson, D.D., Armagh. Monday, 17 th April 1876. Professor FLEEMJNG JENKIN in the Chair. The following Communications were read : — 1. On an Improved Form of Galvanic Battery. By J. Cook, Esq. Communicated by Professor Tail. I wish to direct attention to a simple improvement on battery cells, whereby porous cells are dispensed with, and the incon- veniences of gravity batteries avoided. 149 of Edinburgh, Session 1875-76. I may say it is a year or two since I first tried the plan. It consists in first filling the outer glass cell one-third or one- half with fine silver sand, then pushing a ring of glass (which I cut from a common ale pint-bottle with a hot soldering bolt) down an inch or so into the sand. The zinc element forms a ring round the glass, and the copper lies as a plate on the sand within the glass. Its superiority to the gravity batteries, and to those, such as Sir William Thomson’s, where the sand forms a dividing layer between the copper with its sulphate below and the zinc with its liquid above, will be obvious. I did not find the cupric sulphate solution to diffuse into the zinc division. It so readily admits of inspection that it would be infinitely preferable' to the Meidinger and other plans. 2. On the Properties of the Perigon Yersor. By G. J. P. Grieve, Esq. Communicated by Professor Kelland. 3. Descriptions of some new or imperfectly understood Forms of Palseozoic Corals. By H. Alley ne Nicholson, M.D., D.Sc., F.R.S.E., Professor of Natural History in the University of St Andrews, and James Thomson, F.G.S. (. A bstract). In this communication the authors gave descriptions of several new or imperfectly understood forms of Paheozoic corals. After giving a general account of the method of investigation employed by them, the genus Heliophyllum , Hall, was discussed at length. The external structure of this genus is very peculiar, and it was shown that the genus is not by any means as nearly related to Cyathophyllum as has been generally believed. The new genus Grepidophyllum was proposed for a group of forms possessing the extraordinary and characteristic endothecal dissepiments of Eelio- phyllum, but with the remarkable character that the central tabu- late area of the corallum is shut in by a well-developed accessory wall or inner mural investment. Sometimes this secondary investment constitutes a complete circular sheath to the central tabulate area, and in this case all the primary septa become 150 Proceedings of the Royal Society directly connected with the outer surface of the cylindrical tube thus formed. More commonly, the secondary investment is open all down one side, and becomes directly continuous with two of the primary septa, thus constituting a horse-shoe shaped space, formed by the central tabulate area together with a wide fossula containing three short septa. It was shown that the fine coral described by Mr Billings under the name of Diphyphyllum Archiaci was truly a Crepidophyllum. It was further shown that two different forms, of very similar aspect, had been included by one of the authors under the name of Heliophyllum sub-ccespitosum. One of these forms, the typical one, is a Crepidophyllum, and will stand as G. sub-ccespitosum. The other is a Heliophyllum , and the authors described this under the name of H. elegantulum. The name of Thysanophyllum was proposed for a genus of gestrseiform corals from the Carboniferous rocks of Scotland. This genus is related to Lonsdaleia in the general form of the corallum, in the presence of an exterior vesicular zone of large- sized cells, and in the possession of septa, which have no con- nection with the outer wall. It differs from Lonsdaleia , how- ever, in the fact that the columella, so conspicuous in the latter genus, is wholly wanting, and the central area of the visceral chamber is occupied by strong remote, transverse tabulae. Two species of the genus were described, under the names of Thysano- phyllum orientate and T. minus. Finally, the genus Lindstromia was proposed for a group of small corals, in which the corallum is simple and conical, with an extremely deep calice. The septa are well developed, and meet in the centre of the visceral chamber, where they coalesce to a greater or less extent, and form a strong twisted pseudo-columella, which projects into the floor of the calice, and occupies a large portion of the entire visceral chamber. There are no tabulae, but the septa are furnished with more or less strongly developed dissepiments, which, however, are remote, and do not give rise to any vesicular zone. The genus may, perhaps, be regarded as belonging to the Aporosa. The species L. columnaris was described from the Devonian rocks of North America, and it was mentioned that the authors were in possession of other forms of the genus, still undescribed, from the Carboniferous rocks of Scotland. of Edinburgh, Session 1875-76. 151 4. On a Stable and Flexible Arcb. By Professor Fleeming Jenkin. Monday , May 1876. Professor KELLAND, Vice-President, in the Chair. The Council have awarded the Keith Prize for the biennial period 1873-75, to Professor Crum Brown, for his Re- searches on the Sense of Rotation, and on the Anatomical Relations of the Semi-circular Canals of the Internal Ear. The following Communication was read : — Is the Gaelic Ossian a Translation from the English X By Professor Blackie. The recent revival by a distinguished Celtic scholar of the theory of Laing that Macpherson’s Gaelic Ossian is a translation from the English, affords an opportunity of examining that question in a more strictly philological fashion than it has hitherto had the fortune to enjoy. Parts of the question were no doubt touched by Mackenzie in the Report of the Highland Society, published in 1805 by Graham in his dissertation on the authenticity of Ossian, by Dr Clerk of Kilmalie, the distinguished author of the new version of Ossian in the late splendid edition published at the expense of the Marquis of Bute ; but systematically grappled with the question has never been. Having recently gone through the whole of the originals, I have made careful notes of whatever might tend to settle this question, and have come to the conclusion, in the face of the statement of Mr Campbell — whose authority, no doubt, is one of the highest on the subject, that the Gaelic is unquestionably the original. The tests by which a translator’s hand seems clearly discoverable are the following five: — (1) In the English version, awkward, forced, and unidiomatic expressions frequently occur, which can be clearly traced to the influence of a Gaelic original. (2) In all poems of any antiquity handed down VOL. IX. x 152 Proceedings of the Royal Society in manuscripts, difficulties will occur arising from obsolete words, errors in transcription, confused connection, and other causes. In such cases it is a common practice with translators to skip the diffi- culty, gloss over the matter with some decent commonplace, and sometime to make positive blunders, which is not difficult for a philologer to expose. All these signs of a translator’s hand are frequent in Macpherson’s English, and would be more so bad he not indulged in such a habit of skipping generally that it is difficult to say in certain cases decidedly that the skip was made because the writer of the English wished to shirk a difficulty. (3) It is a common practice with translators, when they find a passage a little obscure, to remove the obscurity by some manifest alteration of the phrase, or even by interpolating a line, or interlarding a com- mentary. This also occurs in Macpherson. (4) It is not always that a translator writes under the same vivid vision, or the same fervid inspiration as the original poet; and the consequence is that he will occasionally degrade poetry into prose, and specially fail to bring out that individuality of character in his word-painting which Ruskin has so triumphantly insisted on in the case of the sister art. The instances of failure to seize the most striking features of the original, and the substitution of generic for specific epithets, are frequent in Macpherson. (5) Most translators y ie — some- times, no doubt, wisely — to the temptation of improving on their originals; and Macpherson, from what we know of him, was the last man in the world to think of resisting such a temptation. How much of the G-aelic, as we now have it — that is, his clean copy of his own originals — was subjected to this process of beauti- fication, as we may call it, no one can now tell, but 1 have traced in several instances departures from the simplicity of the original Gaelic, which can be explained most naturally on the supposition that they proceed from a translator who has yielded, without any just cause, to this flattering seduction. When the results obtained by the detailed application of these tests are combined with the amount of external evidence to be found in the Highland Society’s report to the effect that Macpherson actually did translate from Gaelic originals, and was seen by various parties for weeks and months employed in the work of traslation, a cumulative proof was produced that he was most anxious to see by what arguments Mr 153 of Edinburgh, Session 1875-76. Campbell could rebut. If that gentleman, to whom Celtic litera- ture owes so much (and who in fact is the Wolf of the Ossianic question), or any Galician who thinks with him, shall succeed in leading a counterproof, I can only conclude that, considering the scrappy and fragmentary nature of some of the materials in Mac- pherson’s hands, it might possibly have been the case that the translator filled up some of the gaps in his tale in English, with the intention that they might be done into Gaelic before publica- tion by Strathmaskie, Captain Morrison, or some other of his High- land coadjutors; but that the English, as a whole, is a translation from the Gaelic, and not a translation of the best quality in many respects, may be accepted as one of the best ascertained facts in the whole range of philological investigation. The following Gentlemen were elected Fellows of the Society Professor M. Forster Heddle. J. F. Rodger, S.S.C. William Thomson, F.C.S., Manchester. Monday , Ibth May 1876. Sir WILLIAM THOMSON, President, in the Chair. The Keith Prize for the biennial period 1873-75, which has been awarded to Professor Crum Brown for his Re- searches on the Sense of Rotation, and on the Anatomical Relations of the Semi-circular Canals of the Internal Ear, was presented by the President. The following Communications were read 1. Notes on Dredging in Madeira, by the Rev. Robert Boog Watson, B.A., F.R.S.E., F.G.S. The difficulties in the way of dredging at Madeira are many and considerable. This has probably prevented any of this work having been done since the publication of Mr Macandrew’s list of Mollusca, presented to the British Association in 1854. The author 1 54 Proceedings of the Boyal Society having dredged for several years at Madeira, confirms Macandrew’s generalisation of the Mediterranean character of the Mollusca — excludes 12 of Macandrew’s named list as having crept in by mis- take, and to the 115 remaining species identified by Macandrew as Madeiran has added 200 to 250 more, making nearly 400 in all, of which 80 or perhaps 100 are probably new. These he hopes soon to publish. 2. Note on a New Fossil Foot-Print from the Permian Sandstone of Dumfriesshire. By Patrick Dudgeon, Esq., F.E.S.E. (Plate I.) What appears to be an entirely new foot-print has lately been found in the red sandstone of this district. I have seen many of the foot-prints from the various quarries in the neighbourhood, but have not before observed this one, nor is it like any figured in Sir William Jardine’s splendid work on the “ Ichnology of Annan- dale.” The foot-prints in question were found in a bed about 20 feet from the surface, at Locharbrigg’s Quarry, three miles from Dumfries. They exhibit the usual large hind and smaller fore foot; the impression of the hind foot measures '*5 x 2'’6, the fore foot 2'3 x 1'- 9 ; the stride of the animal appears to have been about 10'. The impression of the hind foot does not interfere with that of the fore foot, as is the case with several of the foot-prints figured in Sir William Jardine’s work, the interval between them being 2' : the hind foot, therefore, must have been put down in the rear of the fore foot when the animal was walking. The impres- sion of the foot shows five toes, the thumb being placed far back. The most characteristic features in these foot-prints are the well- developed claws, and the oblique position of the toes, i.e., they are placed to march one behind the other. In almost all the foot- prints I have seen, where the toes can be made out, the middle one appears the most prominent ; this foot-print is markedly distinct in this respect. As yet I have only been able to obtain one good specimen of this foot-print — a hind foot ; the rest of the slab on which the casts were impressed was unfortunately used for a paving stone in a cottage in the neighbourhood. I got it lifted ; but the rough Proc. Roy Soc.Ednf PlI.Yol.IX. Farlane 2c Erakine . LibkTS EAmT 155 of Edinburgh, Sessio7i 1875-76. usage it had been subjected to had greatly injured the impressions on it ; they were, however, sufficiently distinct to enable me to give the above particulars. The accompanying photograph is a good one of the hind foot in my possession, about half the size of the original. The posterior pad of the foot is not quite complete, and it, together with the pads of the toes, are somewhat broken. I would propose for these foot-prints the provisional name of Herpetichnus loxodactylus , the oblique-toed Herpetichnus, with the following abbreviated character: — Genus Herpetichnus, Jardine (“ Ichnology of Annandale,” 1853, p. 14). Herjpetichnus loxodactylus , sp. nov. Sp. chars. — Fore foot = 2'*3 x l'*9 ; hind foot = 3'‘5 x l/#6 ; stride about 10'; impressions free ; toes 5, oblique; thumb far back; claws well developed. Locality and horizon. — Permian Sandstone, Locharbriggs Quarry, three miles from Dumfries. P.S. — In the discussion which followed this paper, Professor Huxley stated that so far as he could judge from the photograph exhibited, the markings closely resembled a foot-print he had described some years before in a paper read before the Geological Society of London, “ On tbe Stagonolepis Robertsoni (Agassiz) of the Elgin Sandstones ; and on the recently discovered Foot-marks in the Sandstone of Cummingstone ” (“Quart. Jour. Geol. Soc.,” 1859, xv. p. 440). The resemblance of these Cummingstone foot- marks to the Chelichnus of the Dumfriesshire flags was noticed by Professor Huxley in the paper referred to. 3. On the Decennial Period in the Mean Amplitude of the Diurnal Oscillation and Disturbance of the Magnetic Needle and of the Sun-spot Area. By J. A. Broun, F.R.S. (Abstract.) The author, in presenting results relating to the decennial period derived from observations made at Trevandrum during twenty-two years, has sought a redetermination of the mean duration of that 156 Proceedings of the Royal Society period, as shown by preceding magnetical observations connected with bis own. The relation of the frequency and area of sun-spots to the amplitude of the diurnal movements of the magnetic needle gives an increased value to this investigation. Two very different results have been obtained ; — one by Dr Lamont, showing a period of 104 years ; the other, by Dr ft. Wolf, gives 11J years. Dr Lamont’s result depends on the assumption that three periods occurred between 1787 and 1818 — an assump- tion which is opposed to the conclusions which have been deduced from the sun-spot, auroral, and magnetic observations for that interval. Dr Wolfs result has therefore been accepted very gene- rally by many of the most eminent scientific men in England and on the Continent. The author determines the epochs of maximum and minimum range of the diurnal oscillations of the magnetic needle by the more exact method, in which the mean for twelve months corre- sponding (at its middle point) to each month of the year is obtained. Commencing with the Trevandrum observations, from the present time, proceeding backwards to the earliest series, showing a maxi- mum, that of Cassini (Paris 1784-1788.) The maximum at this time (1787'25) is confirmed nearly by Gilpin’s observations (London, 1786-1806). The latter do not show the minimum in 1792 and maximum in 1797, which should satisfy Dr Lamont’s assumption, and they are considered by him, like the observations of sun-spots at the time, as worthless for this investigation. Dr Wolf, on the other hand, finds support in both for a minimum in 1798. It is concluded by the author, from an examination of Gilpin’s observations, that a maximum really happened in 1797*7, but so little marked as to make it probable that any slight corresponding increase of sun-spots would not be noticed by the single, not very accurate, observer at the time. Evidence, however, of a slight maximum is also found in Professor Loomis’s investigation for the frequency of the aurora borealis. As it is certain that another maximum occurred about 1804 to 1806, the author finds that Gilpin’s observations, which agreed with Cassini’s at the commence- ment of the series, showed in all probability the true magnetic variations afterwards. It results from these investigations that the mean duration of the 157 of Edinburgh, Session 1875-76. period is 10-45 years ; but that it appears to undergo a variation between 8 and 12J years in an interval of 42 years. The small maximum of 1797*7, if a true result, may be expected to repeat itself at some future time, a result which could not fail to aid in the search for the cause of these variations. The author shows, that according to the long period of 42 years, a maximum should have happened in 1776 ; but that year Dr Wolf has concluded to be one of minimum sun-spot frequency. That 1776 was really a year of maximum is confirmed by the observa- tions of Van Swinden, who, it is shown, appears to have been the first to obtain a variation due to the decennial period, and to have pointed out the appearance of a law : it is also confirmed by the observations of Cotte at Montmerency. The ratio of the ranges of the diurnal variation in the years when it is a maximum to that in the years of minimum, is com- pared for different parts of the world, and found nearly the same in both hemispheres. It is also found that the law of the diurnal variation is the same in the year of maximum as in the year of minimum. The author concludes that the increase of the diurnal variation is not due to a different cause from that which produces the variation at the minimum, and that this cause acts when there are no sun-spots in the same way as, though with less intensity than, when the latter have their maximum frequency and area. The magnetic variations are therefore not due to the sun-spots ; the latter appearing only when the common cause produces diurnal variations having at least two-thirds of the maximum amplitude. The results derived from the sun-spot area are compared with those from the magnetic observations. While a general agreement is found in the decennial variations from year to year, it is evident that the attempt to calculate the amplitude of the diurnal varia- tion from the sun-spot frequency (as has been done by Dr Wolf) must give results frequently deviating widely from the truth, as might be expected from the previous conclusion. The decennial period of disturbance of magnetic declination at Trevandrum, deduced from hourly observations in the eleven years, 1854 to 1864, is next considered. It is found that the mean disturb- ance at each hour of the day shows the decennial period; but that the range of the mean value, from the minimum to the maximum 158 Proceedings of the Royal Society year, is different for each hour, while the maximum and minimum do not happen at exactly the same time for all hours of the day. Secondary maxima and minima are also shown, which vary in their epochs gradually from midnight to noon. No clear law appears to connect the amount of the maximum disturbance for any hour with that of the minimum for the same hour in the 11 years ; the ratio of the first to the second is least for the hours near noon, and greatest for those near midnight. It is found, however, that the maximum and minimum mean dis- turbance in the diurnal variation for each year, as well as in the decennial variation for each hour, are connected by the following relations : — Dm being the maximum and D0 the minimum dis- turbance. ^/Dm — JD0 = Constant. The monthly mean disturbance at Trevandrum in each of the years 1854 to 1864 is compared with the monthly mean sun-spot areas deduced by Messrs De La Hue, Stewart, and Loewy, from Carrington’s and the Kew Observations, with the following re- sult : — The monthly mean disturbance in the years 1854-56 had a considerable value, and marked variations when there were few or no sun-spots. In 1857 to 1862 there are found several maxima and minima of disturbance and sun-spots which occur simulta- neously. In some cases, and especially in June 1862, there is a well-marked sun-spot area maximum without any corresponding change of magnetic disturbance. The cause of the solar disturb- ance did not then extend its action to the earth at that time. The author concludes with a notice of the hypotheses proposed to explain the decennial period of magnetic variations and of sun- spot frequency, as well as of the cause of sun-spots. It is pointed out that no theory of sun-spot formation can be accepted which does not explain their non- (or very rare) appearance every 10 or 11 years, and therefore the cause of the decennial period is bound up with this explanation. A planetary action which disturbs the equilibrium of the solar gases has been proposed ; no other seems to present itself, and this the author believes will be found ulti- mately to be in question ; and though he has not himself been able to find any satisfactory evidence in its favour, yet remarkable results have been obtained by Messrs De De Eue, Stewart, and Loewy. 159 of Edinburgh , Session 1875-76. 4. On the Parallel Roads of Lockaber. By David Milne Home, LL.D. ( A bstract .) The author referred to the papers written on the subject, begin- ning with that by Dr Macculloch, in the year 1817 ; and he explained the various theories suggested. He intimated his adoption of the Lake theory, and expressed his adherence to the view he took in the memoir read by him in this Society in the year 1846, that the blockages of the lakes had been effected by detrital matter. In support of this view, he pointed out that all over this district of the Highlands there were immense beds of clay, sand, and gravel up to the tops of the hills, at even 2000 feet above the present level of the sea. These deposits he considered to be undeniable proofs of the prevalence of the sea over this part of the earth’s surface to a height of 3000 feet at least. When the sea retired, so as to expose to atmospheric action the higher parts of the country, there would be depressions in the sur- face of the land, where lakes would be formed. These lakes would continue at high levels, till the streams issuing from them cut through the detritus. In some cases, the process of erosion would be so gradual, that the lakes would subside without producing any conspicuous beach-lines on the mountain sides. In other cases, the removal of the blockages would be on a large scale, owing to the looseness of the detritus ; and if these removals were separated from one another by a considerable interval of time, beach-lines of a permanent character would be formed on the sides of the mountains enclosing the valleys. The author referred to the existence in this district of the High- lands, now, of several lakes at high levels, which were kept up by detrital blockages. He instanced, in particular, Loch Earba, in the Lochaber district, at a height of about 1150 feet, which was kept up by such means, and on whose banks there was evidence that the lake had once stood 30 feet higher than at present. Near Kingussie there was Loch Gwynae, at a height of 1015 feet above the sea, on whose sides there were traces of five terraces, the highest of which is 132 feet above the present surface of the lake. VOL. IX. Y 160 Proceedings of the Royal Society He referred to the ample means of cutting through and remov- ing detrital matter possessed by streams and rivers, mentioning particularly the enormous cliffs of detritus cut through by the Rivers Spean and Spey. He next proceeded to discuss the theories of other geologists. With regard to the theory that the parallel roads were formed by the sea, he adduced arguments to show, that this view was im- possible, inasmuch as the “roads” should in that case have all stood at the same level ; whereas, in the different glens, they stood at different levels. Moreover, it had been found, that old river courses existed, by which the water in G-len Gfluoy flowed into the water in Glen Roy, and that the water in Glen Roy flowed through Glen Glaster into Loch Laggan, — a state of things utterly fatal to the marine theory. With regard to the blockage of the lakes having been formed ice , the following objections were stated : — ls£, The improbability that some of the glens were filled with water, whilst others were filled with ice, the temperature of those glens being all much the same, in consequence of nearly equal altitudes above the sea. 2d, The impossibility of getting a glacier to come to the exact spot, where the lakes stopped, to form barriers several miles long, so solid and permanent in structure, as to prevent the escape of the water from lakes above 300 feet deep. The author concluded by referring to the numerous examples in the Lochaber district, of boulders perched on tops of hills, and of rocks smoothed and striated. These phenomena had been ascribed by some geologists to the action of land-ice. But, coupling with these high-perched boulders, the occurrence of kaims or eskars on the sides of the hills (above the parallel roads), and therefore formed before the Lake period, the author was inclined to ascribe these phenomena to one agent — viz., a sea loaded with ice, when the land was submerged, and to a strong current in the sea, from the north-west, which swept over the submerged land, and through such valleys as Glen Spean and Glen Roy. The lakes, he referred to the period when the land was rising out of the sea. Their beaches were formed on the marine detritus; — which also for a time dammed back the lake waters. of Edinburgh, Session 1875-76. 161 Monday , 5th June 1876. D. STEVENSON, Esq., C.E., Vice-President, in the Chair. The following Communications were read : — 1. Physical Observations in Northern Asia. By Professor G. Forbes. 2. On Parallel Motions. By the Rev. John Wilson, M.A., Bannockburn Academy. Communicated by Professor Kelland. It has been well said that the transmission of force is an ‘‘essen- tial condition in machinery.” It is no less true that directness in transference is important; that the fewer links in the chain bind- ing driver and follower together, the less likely is the machine to be put out of gear. There is no question here as to the compara- tive values of the different modes of conveying motion from a prime mover, — rolling contact, sliding contact, wrapping connec- tors, or linkwork. Each has its own excellencies ; each its special advantages ; and one is to be preferred to another only according to the nature of the work to be done. I. Watt's Parallel Motion. — The general problem is the “com- mutation of circular with rectilinear motion.” The importance of the question began to be felt soon after the introduction of the steam-engine; and Watt, in 1784, patented an invention which not only had the credit of being the earliest, but up to recent times, the most reliable and accurate parallel motion in existence. This system was a great advance on the huge chains and arches which were affixed to the working beam of the engine for the pur- pose of obtaining the desired motion; and it has proved to be suf- ficiently accurate for all practical purposes. The construction is simple, consisting of three bars : two, rotating round fixed centres, and connected at their other extremities to the third bar. A point in this bar, either within or without the points of junction, accord- 162 Proceedings of the Royal Society ing as the centres are on opposite sides, or on one side of the con- necting rod, moves in a straight line. The simple explanation of the underlying principle is that the curvature in one direction is modified by the curvature in an opposite direction, due to the motion of the other bar. In both the original and the modified form of this three-bar motion there is a divergence from the straight line, which though inappreciable for small angles, becomes some- what more apparent for larger ones. The determination of the parallel point is given in the formula QF : FP : : AP : BQ In the figures 1 and 2, A.P and BQ are the arms; PQ the con- Fig. 1. Fig. 2. necting link. Let the centres A and B be chosen so that the line mM shall bisect the versed sines of BQ and AP; the throw QK being equal to PT. 163 of Edinburgh, Session 1875-76. 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