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Mechanical energy transportThe 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.
Document ID
19800051398
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Stein, R. F.
(Michigan State University East Lansing, Mich., United States)
Leibacher, J. W.
(Lockheed Research Laboratories Palo Alto, Calif., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Subject Category
Astrophysics
Meeting Information
Meeting: Stellar turbulence
Location: Ontario
Country: Canada
Start Date: August 27, 1979
End Date: August 30, 1979
Accession Number
80A35568
Funding Number(s)
CONTRACT_GRANT: NSG-7293
CONTRACT_GRANT: NSF AST-76-22479
CONTRACT_GRANT: NASW-3053
CONTRACT_GRANT: NAS5-23758
CONTRACT_GRANT: F19678-77-C-0068
Distribution Limits
Public
Copyright
Other

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