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《Acta Physica Sinica》 2005-01
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Analysis of 1991 March 24 CME’s structure using galactic cosmic rays’data

Le Gui-Ming 1)2) Han Yan-Ben 1) 1)(The National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100012,China) 2)(Center for Space Science and Applied Research, Chinese Academy of Sciences,Beijing 100080,China)  
In this paper,1991 March 24 CME's structure is analyzed by determining the moment of sudden change in galactic cosmic ray intensites using wavelet method based on the sudden change in galactic cosmic ray intensities when a CME just arrives at the magnetosphere. The results show that the thickness of the CME-driven shock is about 0.2228AU,while the space scale from the front side of the CME to the most intense magnetic structure is about 0.325AU.
【Fund】: 国家自然科学基金 (批准号 :10 3 73 0 17);; 和国家高技术研究发展计划 (批准号 :2 2 814 4)资助的课题~~
【CateGory Index】: P172.4
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