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Slow mode shocks propagating in open and closed magnetic fields
Lv JY(吕建永); Wei FS(魏奉思); 北京8701信箱
Department空间天气学国家重点实验室
Source PublicationScience in China Series a-Mathematics Physics Astronomy
1999
Volume42Issue:4Pages:414-422
ISSN1006-9283
Language英语
KeywordMhd Simulation Slow Shock Intermediate Shock Solar-wind Waves
AbstractA 2-D MHD model is used to investigate the propagation of slow mode shocks in the open and closed magnetic fields of the meridional plane near the sun. The solutions demonstrate that a forward slow shock could retain its slow shock characteristics into interplanetary space in the magnetically open region; however, it can evolve into an intermediate shock through the helmet-type current sheet to the open magnetic field.
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/122/997
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Lv JY,Wei FS,北京8701信箱. Slow mode shocks propagating in open and closed magnetic fields[J]. Science in China Series a-Mathematics Physics Astronomy,1999,42(4):414-422.
APA 吕建永,魏奉思,&北京8701信箱.(1999).Slow mode shocks propagating in open and closed magnetic fields.Science in China Series a-Mathematics Physics Astronomy,42(4),414-422.
MLA 吕建永,et al."Slow mode shocks propagating in open and closed magnetic fields".Science in China Series a-Mathematics Physics Astronomy 42.4(1999):414-422.
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