Single-fluid 2D magnetohydrodynamic simulation of solar wind structure in comparison to ulysses observations-Reference-Cited by-同舟云学术

Single-fluid 2D magnetohydrodynamic simulation of solar wind structure in comparison to ulysses observations

Published:2000-12 Issue:4 Volume:5 Page:447-450
ISSN:1007-1202
Container-title:Wuhan University Journal of Natural Sciences
language:en
Short-container-title:Wuhan Univ. J. Nat. Sci.

Author:

Ling-yun Deng,Jing-fang Wang,Chang-qing Xiang,Dong-hui Xiong

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://link.springer.com/content/pdf/10.1007/BF02850772.pdf

Reference5 articles.

1. Lu Xian-he, Wei Feng-si. Ulysses Observations and Discussions of Acceleration Mechanisms for the Solar Wind.Chinese J Geophys, 1998,41(4): 437–446.

2. Wang A H, Wu S T. Global Model of the Corona with Heat and Momentum Addition.J Geophys Res, 1998,103: 1913–1922.

3. Habbal S R, Hu Y Q, Esser R. Standing Shocks in a Two-Fluid Solar Wind.J Geophys Res, 1994,99: 8465–8478.

4. Zhang Bei-chen. The Formation of Loop-Like CME and Its Progress in the Inner Solar Space[Wuhan University Doctor's Degree Dissertation.]. Wuhan University: College of Electronic Information, 1997.

5. Phillips J L, Bame S J, Barrackough B L,et al. Ulysses Solar Wind Plasma Observation from Pole to Pole.Geophys Res Lett, 1995,22(23): 3301–3304.

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1. A magnetohydrodynamic simulation of the single-fluid 2-D structure of the solar wind;CHINESE ASTRON ASTR;2003

2. A magnetohydrodynamic simulation of the single-fluid 2-D structure of the solar wind;Chinese Astronomy and Astrophysics;2003-07