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中国物理学会期刊

用银河宇宙线数据分析1991年3月24日CME的结构

CSTR: 32037.14.aps.54.467

Analysis of 1991 March 24 CME’s structure using galactic cosmic rays’ data

CSTR: 32037.14.aps.54.467
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  • 依据CME到达磁层时会引起银河宇宙线强度的突然下降,利用小波分析方法确定宇宙线强度变化的突变时刻,判断CME到达磁层顶的时刻,从而得到这次CME在磁层顶附近的结构.分析结果表明,CME驱动的激波厚度约为02228AU,CME的前端到CME最强磁场结构的空间尺度约为0325AU.

     

    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 sho ck is about 02228AU,while the space scale from the front side of the CME to th e most intense magnetic structure is about 0325AU.

     

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