Magnetospheric Physics in China  

作　　者：CAO Jinbin YANG Junying 

机构地区：[1]Space Science Institute, School of Space and Environment, Beihang University,Beijing 100191

出　　处：《空间科学学报》2018年第5期694-762,共69页Chinese Journal of Space Science

摘　　要：In the past two years, much progress has been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS, RBSP, Swarm, MMS, ARTEMIS, MESSENGER missions etc., or by computer simulations. This paper briefly reviews these works based on papers selected from the 227 publications from January 2016 to December 2017. The subjects cover most sub-branches of magnetospheric physics,including geomagnetic storm, magnetospheric substorm, magnetic reconnection, solar wind-magnetosphereionosphere interaction, radiation belt, plasmasphere, outer magnetosphere, magnetotail, geomagnetic field,auroras, and currents.In the past two years, much progress has been made in magnetospheric physics by using the data of Double Star Program, Cluster, THEMIS, RBSP, Swarm, MMS, ARTEMIS, MESSENGER missions etc., or by computer simulations. This paper briefly reviews these works based on papers selected from the 227 publications from January 2016 to December 2017. The subjects cover most sub-branches of magnetospheric physics,including geomagnetic storm, magnetospheric substorm, magnetic reconnection, solar wind-magnetosphereionosphere interaction, radiation belt, plasmasphere, outer magnetosphere, magnetotail, geomagnetic field,auroras, and currents.

关 键 词：物理 中国 计算机模拟 相互作用 出版物 暴风雨 磁气圈 报纸 

分 类 号：P353[天文地球—空间物理学]