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地球磁场对太阳风扰动响应的研究
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作者 丁留贯 蒋勇 徐飞 《空间科学学报》 CAS CSCD 北大核心 2011年第2期170-175,共6页
分别对行星际激波、太阳风动压增大事件和减小事件的地球磁场响应进行了比较.分析结果表明,同步轨道磁场对太阳风扰动在向阳面产生较强的正响应,在背阳面响应较弱且有时会出现负响应,地磁指数SYM-H对太阳风扰动的响应为正响应.同时还得... 分别对行星际激波、太阳风动压增大事件和减小事件的地球磁场响应进行了比较.分析结果表明,同步轨道磁场对太阳风扰动在向阳面产生较强的正响应,在背阳面响应较弱且有时会出现负响应,地磁指数SYM-H对太阳风扰动的响应为正响应.同时还得出,向阳侧同步轨道磁场响应幅度d B_z与地磁指数响应幅度d SYM-H、上下游动压均方差均具有较好的相关性.地磁指数响应幅度与同步轨道磁场响应幅度相关关系在激波和动压增大事件中具有一致性,动压减小事件出现明显差异,这说明激波和动压增大事件在影响地球磁场方面具有某种共性. 展开更多
关键词 太阳风扰动 动压变化 同步轨道磁场 地磁指数
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Response of magnetic fields at geosynchronous orbit and on the ground to the sudden changes of IMF B_Z 被引量:3
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作者 DONG YiXuan CAO JinBin +2 位作者 LIU WenLong ZHANG Lei LI LiuYuan 《Science China(Technological Sciences)》 SCIE EI CAS 2014年第2期360-367,共8页
The rapid change in the Earth’s magnetosphere caused by solar wind disturbances has been an important part of the solar wind-magnetosphere interaction.However most of the previous studies focused on the perturbation ... The rapid change in the Earth’s magnetosphere caused by solar wind disturbances has been an important part of the solar wind-magnetosphere interaction.However most of the previous studies focused on the perturbation of the Earth’s magnetic field caused by solar wind dynamic pressure changes.In this paper,we studied the response of geosynchronous magnetic field and the magnetic field to the rapid southward turning of interplanetary magnetic field during the interval 1350 1420 UT on 7May 2007.During this event,BZ component of the interplanetary magnetic field decreased from 15 nT to 10 nT within 3 min(1403 1406 UT).The geosynchronous magnetic field measured by three geosynchronous satellites(GOES 10 12)first increased and then decreased.The variations of magnetic field strength in the morning sector(9 10 LT)were much larger than those in the dawn sector(5 LT).Meanwhile,the H components of geomagnetic field on the ground have similar response features but exhibit latitude and LT dependent variations.Compared with H components,the D components do not have regular variations.Although the solar wind dynamical pressure encounters small variations,the magnetic field both in space and on the ground does not display similar variations.Therefore,the increase of geomagnetic field in the dawn sector is caused by the southward turning of IMF(interplanetary magnetic field)BZ.These results will help to better understand the coupling process of geomagnetic filed and interplanetary magnetic field. 展开更多
关键词 interplanetary magnetic field (IMF) solar wind geosynchronous orbit geomagnetic field
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