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Alternative TitleThe simulation of the plasmaspheric morphology during a magnetospheric disturbance event
张华; 徐荣栏; 沈超; 赵华; 北京8701信箱
Source Publication地球物理学报
Keyword等离子层结构 等离子体层顶 模拟 Euv
Other AbstractIn this paper, we have simulated the evolution of the plasmaspheric formation during the geomagnetospheric substorm on 8 to 10 June, 2001. The simulation is based on the mechanism of E×B drift motion of plasmaspheric charged particles in the magnetic equatorial plane. We used the models of Weimer's convection electric field in ionosphere [2001] and Tsyganenko's magnetic field [T96] as the background fields. The results of the simulations have reproduced the structures of plasmaspause, such as plumes, shoulders and channels, which are in consistence with the EUV observations of IMAGE satellite.
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
张华,徐荣栏,沈超,等. 地磁扰动期间等离子体层顶结构的模拟研究[J]. 地球物理学报,2013,56(3):731-737.
APA 张华,徐荣栏,沈超,赵华,&北京8701信箱.(2013).地磁扰动期间等离子体层顶结构的模拟研究.地球物理学报,56(3),731-737.
MLA 张华,et al."地磁扰动期间等离子体层顶结构的模拟研究".地球物理学报 56.3(2013):731-737.
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