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太阳质子事件、双带耀斑及日冕物质抛射
引用本文:李小聪.太阳质子事件、双带耀斑及日冕物质抛射[J].地球物理学进展,1999(Z1).
作者姓名:李小聪
作者单位:中国科学院北京天文台!北京100012
基金项目:中国科学院九五重大基金项目及天文委员会太阳物理分支学科组资助
摘    要:本文统计了第22 太阳活动周期间(1991 ~1995 年) 发生的25 个太阳质子事件与太阳耀斑及日冕物质抛射(CME) 事件的关系  统计结果表明, 所有的太阳质子事件都与耀斑发生相关, 除2 个质子事件(19941020 和19951020 日发生的太阳质子事件) 与CME发生无关, 其余质子事件也都与CME 相关  值得注意的是, 与质子事件相关的耀斑有16 个是双带耀斑, 其中包括与CME无关的2 个事件的耀斑, 占总数的64 %   上述统计结果证实了无论是太阳耀斑, 还是物质抛射, 它们对太阳质子事件的发生同样起着非常重要的作用

关 键 词:太阳质子事件  太阳耀斑  双带耀斑  日冕物质抛射

SOLAR PROTON EVENT,TWO-RIBBON FLARE AND CORONAL MASS EJECTION
LI Xiao-cong.SOLAR PROTON EVENT,TWO-RIBBON FLARE AND CORONAL MASS EJECTION[J].Progress in Geophysics,1999(Z1).
Authors:LI Xiao-cong
Abstract:The relations among solar proton event,solar flares and coronal mass ejection (CME) events were analyzed These solar events were recorded from 1991 to 1995 of the 22nd solar cycle 25 solar proton events were associated with solar flares and 23 of them were associated with CME events It was noticed that 16 flares associated with solar proton events were two-ribbon flares It means that 64% solar proton events studied were associated with two-ribbon flares Above mentioned statistics show that solar flare and coronal mass ejection play important roles in the occurrence of solar proton event And when CME event takes place associated with two-ribbon flare,the probability of occurrence of a solar proton event is higher It is possible that part of CMEs and solar flares may be produced by reconnection of a magnetic field and reconnection of a magnetic field is an important condition for occurrence of solar proton event
Keywords:Solar proton event  Two-ribbon flare  Coronal mass ejection  
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