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Alternative TitleFeature of the Martian Magnetic Field Structure
张艺腾; 李磊; 北京8701信箱
Source Publication空间科学学报
Keyword火星 磁场 磁异常
Other AbstractBased on a single-fluid MHD model, this paper has studied the global magnetic field structure in the near-Mars space, and investigated the influence of the Martian crustal magnetic fields on the magnetic field structure. Mars baw shock, Magnetic Pileup Region are produced when the solar wind flows over Mars.The interplanetary magnetic field lines are curved and `draping' around the planet. The majority of magnetic field lines bypass over two poles, leaving `V shaped' structure in the wake behind Mars. Near the surface of Mars, the local crustal magnetic fields also have noticeable influence on the magnetic field structure. The crustal magnetic fields at different positions,with different intensities form the dissimilar magnetic filed structure and mini-magnetospheres when interacting with the solar wind. The towed mini-magnetosphere and the mini-magnetosphere with open magnetic lines are illustrated in the paper. The local crustal magnetic fields change the morphology of the magnetic field, and accordingly may play an important role in determining the plasma distribution.
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
张艺腾,李磊,北京8701信箱. 火星空间磁场结构特征[J]. 空间科学学报,2009,29(3):257-261.
APA 张艺腾,李磊,&北京8701信箱.(2009).火星空间磁场结构特征.空间科学学报,29(3),257-261.
MLA 张艺腾,et al."火星空间磁场结构特征".空间科学学报 29.3(2009):257-261.
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