An Improved Model of the Jovian Magnetosphere  

An Improved Model of the Jovian Magnetosphere

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作  者:LU Bin CHEN Chu-Xin 

机构地区:[1]Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026

出  处:《Chinese Physics Letters》2014年第3期184-186,共3页中国物理快报(英文版)

基  金:Supported by the National Natural Science Foundation of China under Grant Nos 41374179 and 41121003, and the Knowledge Innovation Program of the Chinese Academy of Sciences under Grant No KZZD-EW-01-4.

摘  要:The Jovian magnetosphere is modulated by the solar wind and centrifugal force. The configuration of the magnetic field in the previous model of the magnetosphere including the centrifugal force is consistent with the observations at low magnetic latitude (Λ〈50°), while there is a substantial difference between the results of the model and the observations at high magnetic latitude (Λ≥50°), especially in the distant magnetotail. Based on the previous model, a new configuration of the Jovian magnetosphere in the night side is suggested by a three-step transformation in this study. The new magnetosphere obtained by the transformation method is flattened in the z-direction and stretched in the x-direction in distant magnetotail, which agree with general knowledge.The Jovian magnetosphere is modulated by the solar wind and centrifugal force. The configuration of the magnetic field in the previous model of the magnetosphere including the centrifugal force is consistent with the observations at low magnetic latitude (Λ〈50°), while there is a substantial difference between the results of the model and the observations at high magnetic latitude (Λ≥50°), especially in the distant magnetotail. Based on the previous model, a new configuration of the Jovian magnetosphere in the night side is suggested by a three-step transformation in this study. The new magnetosphere obtained by the transformation method is flattened in the z-direction and stretched in the x-direction in distant magnetotail, which agree with general knowledge.

分 类 号:P352[天文地球—空间物理学] P185.4[天文地球—地球物理学]

 

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