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The soft X-ray coronal mass ejection above solar limb of 1998 April 23
Chen XJ(陈晓娟); Chen, XJ (reprint author), Chinese Acad Sci, Yunnan Astron Obsev, Kunming 650011, Peoples R China.
发表期刊CHINESE ASTRONOMY AND ASTROPHYSICS
2002-04
卷号26期号:2页码:172-182
DOI10.1016/S0275-1062(02)00055-3
产权排序第1完成单位
收录类别SCI
关键词Solar Activity Solar Corona X-ray Radio Emission
摘要Using the observational materials of SXT/HXT aboard satellite Yohkoh and the Nobeyama Radioheliograph (NoRH) on 1998-04-23, a comprehensive study of the soft X-ray coronal mass ejection (CME) above solar SE limb shows that there were two magnetic dipolar sources (MDSs), one magnetic capacity belt (MCB) between the MDSs, one neutral current sheet (NCS) and some rare activation sources (ASs). When the MCB was changed by the ASs to become a magnetic energy belt (MEB), both mass and energy were concentrated to form the NCS. When the MDSs were connected by the MEB, the NCS was formed and the CME occurred. Mass was ejected not only from the NCS, but also from the whole MEB. The expanding loop of the CME had the two MDSs as footpoints. The top of the loop was always inclined towards the footpoint of the weaker source, and its locus marks the NCS.
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0275-1062
URL查看原文
WOS记录号WOS:000176345300006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]GEOMAGNETIC STORMS ; INTERPLANETARY ; DISTURBANCES ; SUN ; ORIGIN ; MODEL
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/4142
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通讯作者Chen, XJ (reprint author), Chinese Acad Sci, Yunnan Astron Obsev, Kunming 650011, Peoples R China.
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Chen XJ,Chen, XJ . The soft X-ray coronal mass ejection above solar limb of 1998 April 23[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2002,26(2):172-182.
APA 陈晓娟,&Chen, XJ .(2002).The soft X-ray coronal mass ejection above solar limb of 1998 April 23.CHINESE ASTRONOMY AND ASTROPHYSICS,26(2),172-182.
MLA 陈晓娟,et al."The soft X-ray coronal mass ejection above solar limb of 1998 April 23".CHINESE ASTRONOMY AND ASTROPHYSICS 26.2(2002):172-182.
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