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Standing Shocks in the Inner Slow Solar Wind
Li Bo; Chen Yan-Jun; Li Xing; Li, B (reprint author), Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Sch Space Sci & Phys, Weihai 264209, Peoples R China.
Department空间科学部
Source PublicationCHINESE PHYSICS LETTERS
2011
Volume28Issue:5Pages:59601
ISSN0256-307X
Language英语
AbstractWe examine whether the flow tube along the edge of a coronal streamer supports standing shocks in the inner slow wind by solving an isothermal wind model in terms of the Lambert.. function. It is shown that solutions with standing shocks do exist and they exist in a broad area in the parameter space characterizing the wind temperature and flow tube. In particular, streamers with cusps located at a heliocentric distance greater than or similar to 3.2R(circle dot) can readily support discontinuous slow winds with temperatures barely higher than 1 MK.; We examine whether the flow tube along the edge of a coronal streamer supports standing shocks in the inner slow wind by solving an isothermal wind model in terms of the Lambert.. function. It is shown that solutions with standing shocks do exist and they exist in a broad area in the parameter space characterizing the wind temperature and flow tube. In particular, streamers with cusps located at a heliocentric distance greater than or similar to 3.2R(circle dot) can readily support discontinuous slow winds with temperatures barely higher than 1 MK.
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/122/3237
Collection空间科学部
Corresponding AuthorLi, B (reprint author), Shandong Univ, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Sch Space Sci & Phys, Weihai 264209, Peoples R China.
Recommended Citation
GB/T 7714
Li Bo,Chen Yan-Jun,Li Xing,et al. Standing Shocks in the Inner Slow Solar Wind[J]. CHINESE PHYSICS LETTERS,2011,28(5):59601.
APA Li Bo,Chen Yan-Jun,Li Xing,&Li, B .(2011).Standing Shocks in the Inner Slow Solar Wind.CHINESE PHYSICS LETTERS,28(5),59601.
MLA Li Bo,et al."Standing Shocks in the Inner Slow Solar Wind".CHINESE PHYSICS LETTERS 28.5(2011):59601.
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