Theoretical distribution of O+ ions in the Martian magnetosphere
文献类型:会议论文
作者 | Shi, J. K. ; Schwingenschuh, K. ; Zhang, T. L. ; Torkar, K. ; Lichtenegger, H. ; Liu, Z. X. ; Riedler, W. ; Schmidt, R. |
出版日期 | 2001 |
会议名称 | D3 1/C3 3 Symposium of COSPAR Scientific Commission D held at the 33rd COSPAR Scientific Assembly |
会议日期 | 2001 |
会议地点 | Warsaw, Poland |
页码 | 891-896 |
通讯作者 | 北京8701信箱 |
英文摘要 | Considering the magnetic field measurements obtained recently by Mars Global Surveyor and the data on ions in the Martian environment, a model is developed to study the flux distribution of ions originating from the Martian ionosphere along magnetic field lines with different assumed intrinsic moments. Furthermore, the Martian intrinsic moment is deduced. The results show that the intrinsic moment has an influence on the flux distribution of O+ ions, i.e., the stronger the intrinsic moment, the more quickly the flux of O+ ion will decrease with increasing distance from Mars and the lower of the flux of O+ ions will be in the tail. By comparison of the theoretical result in this paper with the observations, the deduced Martian intrinsic moment is about 2 x 10(21) G(.)cm(3). (C) 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved. |
收录类别 | CPCI |
会议网址 | |
会议录 | Advances in Space Research
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会议录出版者 | Elsevier Science Bv |
学科主题 | 空间物理 |
会议录出版地 | AMSTERDAM |
语种 | 英语 |
ISSN号 | 0273-1177 |
源URL | [http://ir.cssar.ac.cn/handle/122/941] ![]() |
专题 | 国家空间科学中心_空间科学部 |
推荐引用方式 GB/T 7714 |
Shi, J. K.,Schwingenschuh, K.,Zhang, T. L.,et al. Theoretical distribution of O+ ions in the Martian magnetosphere[C]. 见:D3 1/C3 3 Symposium of COSPAR Scientific Commission D held at the 33rd COSPAR Scientific Assembly. Warsaw, Poland. 2001. |
入库方式: OAI收割
来源:国家空间科学中心
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