中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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://000173494400010
会议录Advances in Space Research
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.://000173494400010.

入库方式: OAI收割

来源:国家空间科学中心

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