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关于IMF北向分量特强时的太阳风-磁层-电离层耦合
引用本文:沈长寿 资民筠. 关于IMF北向分量特强时的太阳风-磁层-电离层耦合[J]. 空间科学学报, 1994, 14(1): 76-80. DOI: 10.11728/cjss1994.01.076
作者姓名:沈长寿 资民筠
作者单位:1.北京大学地球物理系, 100871
摘    要:

关 键 词:行星际磁场   太阳风-磁层能量耦合函数
收稿时间:1992-06-12

ON THE SOLAR WIND-MAGNETOSPHERE COUPLING WHEN IMF IS NORTHWARD AND Bz>10 nT
Affiliation:1.Department of Geophysics, Peking University, Beijing 1008712.The Academy of Arts of China, Beijing
Abstract:Relationship between the solar wind-magnetosphere energy coupling function and the energy consumption in the magnetospheric system is tested by the samples during period of northward Bz(>10 nT) of IMF. It is shown that the energy function which can well describe the solar wind-magnetosphere coupling when Bz>0 is no more applicable for Bz>10 nT, but the coupling still exists, the effects of which are mainly found at the polar cap. Dst often turns to positive when Bz> 10 nTand the coupling mechanism is different from that when Bz<0. New coupling function has to be introduced to describe the solar wind-magnetosphere coupling for the case of Bz> 10 nT. 
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