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首页> 外文会议>COSPAR colloquium >CORONAL MASS EJECTIONS: RELATIONSHIP WITH SOLAR FLARES AND CORONAL HOLES
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CORONAL MASS EJECTIONS: RELATIONSHIP WITH SOLAR FLARES AND CORONAL HOLES

机译：冠状大众射血：与太阳能耀斑和冠状孔的关系

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The Coronal Mass Ejections (CMEs) observed by the LASCO coronagraph and associated solar activity phenomena whose locations were identified by EIT and solar Hα flare observations during year 2000 indicate that about 40%, 26% and 30% of CMEs were observed when there were coronal holes (CHs) within 1-10, 11-20 and 21-40 degrees, respectively from the location of solar Hα flares. We are of the view, as also earlier suggested by Verma & Pande (1989), that CMEs might have been produced by the same mechanism by which the mass ejected by the same solar flares or active prominences connects with open magnetic lines of CHs (source of high speed solar wind streams) and moves along them to appear as CMEs.
机译：由Lasco Coronagraphy观察到的冠状大气射出量（CMES），其在2000年期间通过EIT和太阳Hα眩光观测鉴定的位置，表明当冠状冠的情况下，观察到约40％，26％和30％的CMES分别从太阳能Hα耀斑的位置1-10,11-20和21-40度内的孔（CHS）。我们的观点是verma＆pande（1989）建议的，即CMES可能已经通过相同的机制制造，通过相同的太阳耀斑或有源突出的质量与CHS的开放磁线连接（来源）高速太阳风流）并沿着它们移动以显示为CMES。

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