SUPRATHERMAL SOLAR WIND ELECTRONS AND LANGMUIR TURBULENCE

ASTROPHYSICAL JOURNAL, pp. 602016.

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Abstract:

The steady-state model recently put forth for the solar wind electron velocity distribution function during quiet time conditions, was originally composed of three population electrons (core, halo, and superhalo) with the core remaining nonresonant with any plasma waves while the halo and superhalo separately maintained steady-state reson...More

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