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远磁尾磁层顶位形的偏转

商文赛 吕建永 王明 倪素兰

商文赛, 吕建永, 王明, 倪素兰. 远磁尾磁层顶位形的偏转[J]. 空间科学学报, 2018, 38(3): 307-314. doi: 10.11728/cjss2018.03.307
引用本文: 商文赛, 吕建永, 王明, 倪素兰. 远磁尾磁层顶位形的偏转[J]. 空间科学学报, 2018, 38(3): 307-314. doi: 10.11728/cjss2018.03.307
SHANG Wensai, LÜ Jianyong, WANG Ming, NI Sulan. Deflection of Magnetopause in the Distant Magnetotail[J]. Chinese Journal of Space Science, 2018, 38(3): 307-314. doi: 10.11728/cjss2018.03.307
Citation: SHANG Wensai, LÜ Jianyong, WANG Ming, NI Sulan. Deflection of Magnetopause in the Distant Magnetotail[J]. Chinese Journal of Space Science, 2018, 38(3): 307-314. doi: 10.11728/cjss2018.03.307

远磁尾磁层顶位形的偏转

doi: 10.11728/cjss2018.03.307
基金项目: 

国家自然科学基金项目(41574158,41604141,U1631107),江苏省双创(2014)人才项目,江苏省研究生培养创新工程(KYLX15_0877)和江苏省自然科学青年基金项目(BK20160952)共同资助

详细信息
    作者简介:

    吕建永,E-mail:jylu@nuist.edu.cn;商文赛,E-mail:wensaishang@163.com

  • 中图分类号: P353

Deflection of Magnetopause in the Distant Magnetotail

  • 摘要: 利用WIND和ARTEMIS卫星观测数据,分析远磁尾磁层顶对行星际和太阳风变化的响应,尤其是偏离日地连线的太阳风速度改变对远磁尾磁层顶的影响.研究发现在2011年9月13日的事件中,P2卫星观测到高速且高密度的磁鞘流.利用最小变量法进行分析发现,磁层顶沿着偏离日地连线的太阳风速度方向发生偏转.根据相似三角形定理,推断出本次事件中磁层顶在y方向和z方向上的偏转幅度分别达到10Re和6Re.P1和P2卫星的相对位置也证实了这一观点.因此,偏离日地连线的太阳风速度对远磁尾磁层顶的位形影响很大.研究结果可为建立包含太阳风速度vyvz效应的磁层顶模型提供观测证据.

     

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出版历程
  • 收稿日期:  2017-04-06
  • 修回日期:  2017-10-03
  • 刊出日期:  2018-05-15

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