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强磁场扰动对宇宙线调制的统计研究
引用本文:郭维吉, 章公亮. 强磁场扰动对宇宙线调制的统计研究[J]. 空间科学学报, 1995, 15(4): 295-300. doi: 10.11728/cjss1995.04.295
作者姓名:郭维吉 章公亮
作者单位:中国科学院空间科学与应用研究中心, 北京 100081
基金项目:国家自然科学基金,青年基金
摘    要:对1978─1982太阳活动高年时发生的激波、强磁场扰动及激波与强磁场扰动共存这三类事件引起的宇宙线变化进行了统计研究,得到如下结果:(1)激波与强磁场扰动共存时引起的宇宙线强度下降最为显着;只有激波或强磁场扰动时,宇宙线的强度变化相对较小;(2)标志速度间断的激波是产生宇宙线Forbush下降的重要因素;(3)速度间断在强磁场扰动对宇宙线的调制中可能起一个触发的作用。

关 键 词:速度间断   激波   强磁场扰动   宇宙线调制
收稿时间:1994-10-19
修稿时间:1900-01-01

STATISTICAL STUDY OF CSOMIC RAY MODULATION PRODUCED BY INTERPLANETARY STRONG MAGNETIC FIELD DISTURBANCE
Guo Wei-ji, Zhang Gong-liang. STATISTICAL STUDY OF CSOMIC RAY MODULATION PRODUCED BY INTERPLANETARY STRONG MAGNETIC FIELD DISTURBANCE[J]. Chinese Journal of Space Science, 1995, 15(4): 295-300. doi: 10.11728/cjss1995.04.295
Authors:Guo Wei-ji  Zhang Gong-liang
Affiliation:Center for Space Science and Applied Research, Academia Sinica, Beijing 100080
Abstract:Three categories of interplanetary disturbances have been chosen from the period 1978--1982 when solar activity was high. They are:(i)shock wave;(ii)strong magnetic field disturbance;(iii)strong magnetic field disturbance behind shock wave. The cosmic ray variations produced by them have been studied statistically.The following results are obtained:(1)cosmic ray decrease resulted from the strong magnetic field disturbance is very obvious when there is a shock wave before it,but the cosmic ray decrease is relatively small when only shock wave or strong magnetic disturbance exists;(2)the shock wave which indicates the speed discontinuity is a vital factor resulting the Forbush decrease;(3)the speed discontinuity may take a role of trigger in the process of the cosmic ray modulation produced by the strong magnetic field disturbance.
Keywords:speed discontinuity  shock wave  strong magnetic field disturbance  cosmic ray modulation  
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