Effect of coupled electron-proton thermal conductivities on the two-fluid solutions for the quiet solar wind
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 11 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY;The Astrophysical Journal;2014-05-20
2. ON THE COMPETITION BETWEEN RADIAL EXPANSION AND COULOMB COLLISIONS IN SHAPING THE ELECTRON VELOCITY DISTRIBUTION FUNCTION: KINETIC SIMULATIONS;The Astrophysical Journal;2012-11-16
3. A fast solar wind model with anisotropic proton temperature;Journal of Geophysical Research: Space Physics;1997-01
4. An eight-moment approximation two-fluid model of the solar wind;Journal of Geophysical Research: Space Physics;1996-07-01
5. Latitudinal variations in the solar wind electron heat flux;Space Science Reviews;1995-04
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