Three-fluid solar wind model with Alfven waves

Details Three-fluid solar wind model with Alfven waves Three-fluid solar wind model with Alfven waves

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995sowi.conf...64e&link_type=abstract

Harvard-Smithsonian Center for Astrophysics, International Solar Wind 8 Conference, p. 64

Mathematics

Solar Wind, Magnetohydrodynamic Waves, Proton Energy, Electron Energy, Alpha Particles, Plasma Heating, Flow Characteristics, Solar Corona, Stellar Models, Continuity (Mathematics), Momentum, Kinetic Energy, Heat Sources

Scientific paper

We 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.

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