Title of article
Theoretical distribution of O+ ions in the martian magnetosphere Original Research Article
Author/Authors
J.K. Shi، نويسنده , , K. Schwingenschuh، نويسنده , , T.L. Zhang، نويسنده , , K. Torkar، نويسنده , , H. Lichtenegger، نويسنده , , Z.X. Liu، نويسنده , , W. Riedler، نويسنده , , R. Schmidt، نويسنده , , C.P Escoubet، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2001
Pages
6
From page
891
To page
896
Abstract
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 2×1021G·cm3.
Journal title
Advances in Space Research
Serial Year
2001
Journal title
Advances in Space Research
Record number
1127686
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