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Theoretical distribution of O+ ions in the Martian magnetosphere
Shi, J. K.; Schwingenschuh, K.; Zhang, T. L.; Torkar, K.; Lichtenegger, H.; Liu, Z. X.; Riedler, W.; Schmidt, R.; 北京8701信箱
Department空间天气学国家重点实验室
Source PublicationAdvances in Space Research
2001
Pages891-896
Language英语
ISSN0273-1177
AbstractConsidering 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.
Conference NameD3 1/C3 3 Symposium of COSPAR Scientific Commission D held at the 33rd COSPAR Scientific Assembly
Conference Date2001
Conference PlaceWarsaw, Poland
Indexed ByCPCI
Document Type会议论文
Identifierhttp://ir.nssc.ac.cn/handle/122/941
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Shi, J. K.,Schwingenschuh, K.,Zhang, T. L.,et al. Theoretical distribution of O+ ions in the Martian magnetosphere[C]. AMSTERDAM:Elsevier Science Bv,2001:891-896.
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