STEADY-STATE MODEL OF SOLAR WIND ELECTRONS REVISITED
ASTROPHYSICAL JOURNAL, pp. 1692015.
In a recent paper, Kim et al. put forth a steady-state model for the solar wind electrons. The model assumed local equilibrium between the halo electrons, characterized by an intermediate energy range, and the whistler-range fluctuations. The basic wave-particle interaction is assumed to be the cyclotron resonance. Similarly, it was assum...More
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