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《Chinese Journal of Geophysics》 1994-S2
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THE ENERGY INPUT TO THE MAGNETOSPHERIC SYSTEM AND THE SOLAR-TERRESTRIAL COUPLING

ZI MIN-YUN(The Academy of Arts of China, Beijing 100009)SHEN CHANG-SHOU(Department of Geophysical,Peking University,Beijing 100871)  
The data of solar wind,IMF and geomagnetic field of 36 geomagnetic storms in 1978 and 1982 are used to test the two kinds of the solar wind-magnetosphere energy coupling function.The results indicate that the coupling function presented by Akasofu can be used to predict roughly the occurrence of geomagnetic substorm and storm,but instead of a simple linear correlation,It is a logarithmic linear relationship between εand the consumption of the magnetospheric system.A substorm will occur when e starts to play an important role.When the energy consumption in the ionosphere attends its saturated value,a geomagnetic storm will apPear.Using geomagnetic data from 1978 to 1986,the 27-day distribution of the energy consumption in the ring current and in the auroral ionosphere is alsc calculated.It is likely that similar to the earth seismic belt,there are some long listing active areas on the solar disk.
【Fund】: 国家自然科学基金
【CateGory Index】: P318
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