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宇宙线暴时增加及其特征
引用本文:叶宗海,孙小青.宇宙线暴时增加及其特征[J].空间科学学报,1992,12(4):270-278.
作者姓名:叶宗海  孙小青
作者单位:中国科学院空间科学与应用研究中心,中国科学院空间科学与应用研究中心 北京 100080,北京 100080
摘    要:利用11个地面超中子堆的资料分析了6个不同地磁暴期间由于赤道环电流增强引起的暴时增加,并分析了它们的特征。结果表明,地磁暴愈强,暴时增加愈明显。暴时增加与地磁H分量的变化有很好的负相关,并有明显的纬度效应或与地磁截止刚度有依赖关系。北京地区是暴时增加相当明显的区域。暴时增加还有明显的地方时依赖关系。在白昼一侧的增加更大,表明环电流具有不对称性的特征。

关 键 词:宇宙线  暴时增加  环电流  地磁暴

STORM-TIME INCREASE IN COSMIC RAY INTENSITY AND ITS CHARACTERISTICS
Ye Zong-hai Sun Xiao-qing.STORM-TIME INCREASE IN COSMIC RAY INTENSITY AND ITS CHARACTERISTICS[J].Chinese Journal of Space Science,1992,12(4):270-278.
Authors:Ye Zong-hai Sun Xiao-qing
Abstract:The cosmic ray increases due to considerable depressions of cosmic ray cut off rigidity during large geomagnetic storms are investigated.Data from 11 superneutron monitors in world network are analyzed for six geomagnetic storms of various type during 1984-1989.The results show that the storm-time increases are due to existence of westward equatorial ring currents developing or intensifying during geomagnetic storms.The stronger the geomagnetic storm,the larger the storm-time increase.The storm-time increases have obvious latitude effect or geomagnetic cut off rigidity dependence.Beijing station is at the obvious region for the storm-time increase,and storm-time increases are of local tune dependence.This enhancement is larger at the daytime than at the nighttime.Showing that the intensifying ring current is asymmetrical.
Keywords:Cosmic ray Forbush decrease  Storm-time increase  Ring current  Geomagnetic storm
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