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Three-fluid solar wind model with Alfven wavesWe present a study of a three-fluid solar wind model. with continuity, momentum and separate energy equations for protons. alpha particles and electrons. Allowing separate coronal heat sources for all three species, we study the flow properties of the solar wind as a function of heat input, Alfven wave energy input, and alpha particle abundance.
Document ID
19960021363
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Esser, Ruth (Harvard-Smithsonian Center for Astrophysics Cambridge, MA United States)
Habbal, Shadia R. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA United States)
Hu, You Q. (China Scientific and Technical Univ. Hofei, China)
Date Acquired
August 17, 2013
Publication Date
June 30, 1995
Subject Category
Solar Physics
Accession Number
96N24759
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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