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Turbulent Eddy Viscosity and Large-Scale Convection in the Sun

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Turbulent Eddy Viscosity and Large-Scale Convection in the Sun

by
Stothers, Richard B

Publication date
Usage
Public DomainCreative Commons Licensepublicdomain
Topics
CIRRUS CLOUDS, CRYSTALS, ICE, RADIOMETERS, SUBMILLIMETER WAVES, DC 8 AIRCRAFT, MECHANICAL ENGINEERING, WATER VAPOR, SENSITIVITY, BRIGHTNESS TEMPERATURE
Collection
nasa_techdocs
Contributor
NASA
Language
English
Rights
Public Domain
It is suggested here that the laminar character of the large-scale deep convective flows appearing in numerical simulations of the Sun's convective envelope arises from the effect of turbulent eddy viscosity. Previously, M. Schwarzchild suggested the same idea to explain the observed surface granulation in the Sun.
Addeddate
2011-05-29 01:13:42
Document-source
CASI
Documentid
20000057312
Identifier
nasa_techdoc_20000057312
Identifier-ark
ark:/13960/t8cg0kx7r
Nasa-center
Goddard Space Flight Center
Ocr
ABBYY FineReader 8.0
Online-source
http://wayback.archive-it.org/1792/20100216211845/http://hdl.handle.net/2060/20000057312
Original-nasa-rights
Unclassified; No Copyright; Unlimited; Publicly available;
Ppi
300
Updated-added-to-ntrs
2009-05-11
Year
2000

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