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Title: |
Mechanical energy transport
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Author(s): |
Stein, R. F.; Leibacher, J. W.
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Abstract: |
The properties, generation, and dissipation mechanisms of acoustic, gravity and Alfven waves are described, whose restoring forces are pressure, buoyancy, and magnetic tension, respectively. For acoustic waves, generation by turbulent convective motions and by the Eddington Valve thermal overstability is discussed, considering the 'five-minute' oscillation; dissipation is possible either by radiation or shocks. Generation of gravity waves by penetrative convective motions and by shear arising from supergranule motions is reviewed, and dissipation due to wave breaking, interaction with the mean horizontal fluid flow, and very severe radiative damping is considered. Attention is given to Alfven wave generation by convective motions and thermal overstability, and to dissipation by mode coupling, wave decay, current dissipation, and particle collisions producing Joule or viscous heating.
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NASA Center: |
NASA (non Center Specific)
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Publication Date: |
JAN 1, 1980
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Document Source: |
Other Sources |
No Digital Version Available: |
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Document ID: |
19800051398
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Accession ID: |
80A35568
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Publication Information: |
Number of Pages = 23 |
Contract-Grant-Task Number: |
F19678-77-C-0068 |
Meeting Information: |
Stellar turbulence, August 27-30, 1979, Ontario, Canada |
Keywords: |
ATMOSPHERIC TURBULENCE; CONVECTIVE FLOW; ENERGY DISSIPATION; ENERGY TRANSFER; STELLAR ATMOSPHERES; TRANSPORT THEORY; COUPLED MODES; GRAVITY WAVES; LOW LEVEL TURBULENCE; MAGNETOHYDRODYNAMIC WAVES; PARTICLE COLLISIONS; RESISTANCE HEATING; SOUND WAVES;
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Notes: |
In: Stellar turbulence; Proceedings of the Fifty-first Colloquium, London, Ontario, Canada, August 27-30, 1979. (A80-35551 14-90) Berlin and New York, Springer-Verlag, 1980, p. 225-247. Research supported by the Lockheed Independent Research Fund |
Accessibility: |
Unclassified; Copyright; Unlimited; Publicly available; |
Updated/Added to NTRS: |
2004-11-03 |
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