Ideal MHD instabilities for coronal mass ejections Interacting current channels and particle acceleration

被引：0
|
作者：
Keppens, Rony [1 ]
Guo, Yang [2 ]
Makwana, Kirit [3 ]
Mei, Zhixing [4 ]
Ripperda, Bart [5 ]
Xia, Chun [6 ]
Zhao, Xiaozhou [7 ]
机构：
[1] Centre for mathematical Plasma Astrophysics, KU Leuven, Leuven,3001, Belgium
[2] School of Astronomy and Space Science, Nanjing University, Nanjing,210023, China
[3] Deutsches Elektronen-Synchrotron DESY, Platanenallee 6, Zeuthen,D-15738, Germany
[4] Yunnan Observatories, Chinese Academy of Sciences, Kunming, China
[5] Institut fur Theoretische Physik, Max-von-Laue-Str. 1, Frankfurt,D-60438, Germany
[6] Yunnan University, School of Physics and Astronomy, Kunming, China
[7] Purple Mountain Observatory, Nanjing, China
来源：
arXiv | 2019年
关键词：
615.3 Magnetohydrodynamics (MHD) Power Generation - 657.2 Extraterrestrial Physics and Stellar Phenomena - 801.3 Colloid Chemistry - 802.3 Chemical Operations - 921 Mathematics;
D O I：
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中图分类号：
学科分类号：
摘要：
Phase space methods
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