Solar Wind Electron Transport: Interplanetary Electric Field and Heat Conduction
作者： Viviane Pierrard
DOI: 10.1007/S11214-011-9743-6
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摘要: The presence of suprathermal electrons has important consequences on the acceleration process solar wind: they increase electrostatic potential between corona and interplanetary space accelerate wind to high bulk velocities. Moreover, modify heat conduction can explain sharp temperature in corona. These are well evidenced kinetic approach where no closure requires distributions be nearly Maxwellians.
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