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Model for energy transfer in the solar wind: Formulation of modelThe two-fluid solar-wind model is extended by including the collisionless dissipation of hydromagnetic waves originating at the sun. A series of solar wind models is generated, parameterized by the total energy flux of hydromagnetic waves at the base of the model. The resulting properties of propagation and dissipating of hydromagnetic waves on this model are presented.
Document ID
19730002055
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hartle, R. E. (NASA Ames Research Center Moffett Field, CA, United States)
Barnes, A. A., Jr. (NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Publication Information
Publication: Solar Wind
Subject Category
Space Radiation
Accession Number
73N10782
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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