中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Modeling the resistive MHD by the CESE method

文献类型:期刊论文

作者Feng XS(冯学尚) ; Hu YQ(呼延奇) ; Wei FS(魏奉思)
刊名Solar Physics
出版日期2006
卷号235期号:40180页码:235-257
关键词time conservation element euler equations magnetohydrodynamics reconnection
ISSN号0038-0938
通讯作者北京8701信箱
英文摘要In this paper, the Space-Time Conservation Element and Solution Element (CESE) method is applied to 2.5-dimensional resistive magnetohydrodynamics (MHD) equations in Cartesian coordinates, with the purpose of modeling the magnetic reconnection study. To show the validity and capacity of its application to MHD reconnection problem, spontaneous fast reconnection and magnetic reconnection in multiple heliospheric current sheets are studied, which show good consistency with those obtained formerly by other authors. In order to assess the del . B = 0 constraint numerically, the contours and evolution of del.B are analyzed. The numerical results tell us that the CESE numerical scheme not only has good numerical resolution but also can keep the divergence-free condition for magnetic fields in the reconnection problems during the evolutionary process without any special treatment.
学科主题空间物理
收录类别SCI
原文出处http://www.springerlink.com/content/83228235q81555p1/fulltext.pdf
语种英语
源URL[http://ir.cssar.ac.cn/handle/122/1065]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Feng XS,Hu YQ,Wei FS. Modeling the resistive MHD by the CESE method[J]. Solar Physics,2006,235(40180):235-257.
APA 冯学尚,呼延奇,&魏奉思.(2006).Modeling the resistive MHD by the CESE method.Solar Physics,235(40180),235-257.
MLA 冯学尚,et al."Modeling the resistive MHD by the CESE method".Solar Physics 235.40180(2006):235-257.

入库方式: OAI收割

来源:国家空间科学中心

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