Acceleration and heating of two-fluid solar wind by Alfven waves
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 15 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. Coronal heating and acceleration of the high/low-speed solar wind by fast/slow MHD shock trains;Monthly Notices of the Royal Astronomical Society;2004-04
3. A two-dimensional Alfvén wave–driven solar wind model with proton temperature anisotropy;Journal of Geophysical Research;2004
4. A model for the jet-disk connection in BH accreting systems;Astronomy & Astrophysics;2003-09
5. On the Heating of the Solar Corona and the Acceleration of the Low‐Speed Solar Wind by Acoustic Waves Generated in the Corona;The Astrophysical Journal;2002-10-10
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