中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
PROPAGATION OF SOLAR FLARE-ASSOCIATED INTERPLANETARY SHOCK-WAVES IN THE HELIOSPHERIC MERIDIONAL PLANE

文献类型:期刊论文

作者Wei, F. S. ; Dryer, M.
刊名Solar Physics
出版日期1991
卷号132期号:2页码:373-394
关键词ips observations august 1972 wind speed disturbances scintillation
ISSN号0038-0938
通讯作者北京8701信箱
英文摘要We have analyzed 149 flare-associated shock wave events based on interplanetary scintillation (IPS) observational data. All of the flare-associated shock waves tend to propagate toward the low latitude region near the solar equator for flares that are located in both the solar northern and southern hemispheres. Also, the fastest propagation directions tend toward the heliospheric current sheet near 1 AU. We suggest that this tendency is caused by the dynamic action of near-Sun magnetic forces on the ejected coronal plasma that traverses the helmet-like magnetic topologies near the Sun outward to the classical topology that is essentially parallel to the heliospheric current sheet.
学科主题空间物理
收录类别SCI
原文出处://A1991FH72900013
语种英语
源URL[http://ir.cssar.ac.cn/handle/122/982]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Wei, F. S.,Dryer, M.. PROPAGATION OF SOLAR FLARE-ASSOCIATED INTERPLANETARY SHOCK-WAVES IN THE HELIOSPHERIC MERIDIONAL PLANE[J]. Solar Physics,1991,132(2):373-394.
APA Wei, F. S.,&Dryer, M..(1991).PROPAGATION OF SOLAR FLARE-ASSOCIATED INTERPLANETARY SHOCK-WAVES IN THE HELIOSPHERIC MERIDIONAL PLANE.Solar Physics,132(2),373-394.
MLA Wei, F. S.,et al."PROPAGATION OF SOLAR FLARE-ASSOCIATED INTERPLANETARY SHOCK-WAVES IN THE HELIOSPHERIC MERIDIONAL PLANE".Solar Physics 132.2(1991):373-394.

入库方式: OAI收割

来源:国家空间科学中心

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