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3D global simulation of the interaction of interplanetary shocks with the magnetosphere
Wang, C.; Huang, Z. H.; Hu, Y. Q.; Guo, X. C.; 北京8701信箱
Department空间天气学国家重点实验室
Source PublicationAip Conference Proceedings
2005
Pages320-324
Language英语
ISSN0094-243X
ISBN0-7354-0268-X
AbstractUsing the recently developed PPMLR-MHD code, we present 3D global simulation of the interaction of the interplanetary(IP) shock with the magnetosphere with emphasis on the the effect of shock orientation. We investigate its impact on the sudden commencement(SC) of geomagnetic storms and the magnetospheric responses. Generally speaking, a highly oblique shock causes asymmetric compression of the magnetosphere with respect to the noon-midnight meridian, and requires more time to compress the forward part of the magnetosphere, which producing longer rise time of SC. Even if the solar wind dynamic pressure changed similarly at a solar wind monitor, the responses of the magnetosphere could vary depending on the orientation of the causative IP shock. The effect of the shock orientation is of great help to understand space weather processes.
KeywordShock Interaction Numerical Simulation
Conference Name4th Annual IGPP International Astrophysics Conference
Conference Date2005
Conference PlacePalm Springs, CA
Indexed ByCPCI
Document Type会议论文
Identifierhttp://ir.nssc.ac.cn/handle/122/947
Collection空间科学部
Corresponding Author北京8701信箱
Recommended Citation
GB/T 7714
Wang, C.,Huang, Z. H.,Hu, Y. Q.,et al. 3D global simulation of the interaction of interplanetary shocks with the magnetosphere[C]. MELVILLE:Amer Inst Physics,2005:320-324.
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