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Modeling the resistive MHD by the CESE method
Feng XS(冯学尚); Hu YQ(呼延奇); Wei FS(魏奉思); 北京8701信箱
Department空间天气学国家重点实验室
Source PublicationSolar Physics
2006
Volume235Issue:40180Pages:235-257
ISSN0038-0938
Language英语
KeywordTime Conservation Element Euler Equations Magnetohydrodynamics Reconnection
AbstractIn 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.
Indexed BySCI
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1065
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Feng XS,Hu YQ,Wei FS,et al. 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,&北京8701信箱.(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.
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