Ring current modeling in a realistic magnetic field configuration

被引:76
作者
Fok, MC
Moore, TE
机构
[1] Universities Space Res. Association, Space Sciences Laboratory, NASA/MSFC, Huntsville, AL
[2] Space Sciences Laboratory, NASA/Marshall Space Flight Center, Huntsville, AL
[3] USRA, Space Sciences Laboratory, NASA/MSFC, Huntsville
[4] Space Science Laboratory, ES83, NASA/MSFC, Huntsville
关键词
D O I
10.1029/97GL01255
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A 3-dimensional kinetic model has been developed to study the dynamics of the storm time ring current in a dipole magnetic field. In this paper, the ring current model is extended to include a realistic, time-varying magnetic field model. The magnetic field is expressed as the cross product of the gradients of two Euler potentials and the bounce-averaged particle drifts are calculated in the Euler potential coordinates. A dipolarization event is modeled by collapsing a tail-like magnetosphere to a dipole-like configuration. Our model is able to simulate the sudden enhancements in the ring current ion fluxes and the corresponding ionospheric precipitation during the substorm expansion.
引用
收藏
页码:1775 / 1778
页数:4
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