REVISED MODEL OF THE STEADY-STATE SOLAR WIND HALO ELECTRON VELOCITY DISTRIBUTION FUNCTION
ASTROPHYSICAL JOURNAL, pp. 2042016.
A recent study discussed the steady-state model for solar wind electrons during quiet time conditions. The electrons emanating from the Sun are treated in a composite three-population model-the low-energy Maxwellian core with an energy range of tens of eV, the intermediate similar to 10(2)-10(3) eV energy-range ("halo") electrons, and the...More
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