NASA NTRS · 19960021363
Three-fluid solar wind model with Alfven waves
Abstract
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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Esser, Ruth, Habbal, Shadia R., Hu, You Q.. 1995-06-30. Three-fluid solar wind model with Alfven waves. https://ntrs.nasa.gov/citations/19960021363
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