Recent progress in MHD simulations of the solar-terrestrial connection
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Engineering,General Materials Science
Link
http://link.springer.com/content/pdf/10.1007/s11431-015-5992-z.pdf
Reference10 articles.
1. Gressl C, Veronig A M, Temmer M, et al. Comparative study of MHD modeling of the background solar wind. Solar Phys, 2014, 289, 1783
2. Oran R, van der Holst B, Landi E, et al. A global wave-driven magnetohydrodynamic solar model with a unified treatment of open and closed magnetic field topologies. Astrophys J, 2013, 778, 176
3. Feng X S, Zhong D K, Xiang C Q, et al. GPU-accelerated computing of three-dimensional solar wind background, Sci China Earth Sci, 2013, 56, 11: 1864–1880
4. Zhou Y F, Feng X S. An improved CESE method and its application to steady-state coronal structure simulation. Sci China Earth Sci, 2014, 57: 153–166
5. Zhou Y F, Feng X S, Zhao X H. Using a 3-D MHD simulation to interpret propagation and evolution of a coronalmass ejection observed by multiple spacecraft: The 3 April 2010 event. J Geophys Res Space Phys, 2014, 119: 9321–9333
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