Cluster of solar active regions and onset of coronal mass ejections

查看全文 作　　者：WANG [1]JingXiu;ZHANG [1]YuZong;HE [1]Han;CHEN [2]AnQin;JIN [1]ChunLan;ZHOU [1]GuiPing

机构地区：[1]Key Lab of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences;[2]National Center for Space Weather,China Meteorological Administration

出　　处：《Science China(Physics,Mechanics & Astronomy)》索引2015年第58卷第9期,共8页

基　　金：supported by the National Natural Science Foundation of China(Grant Nos.11221063,11373004,11322329,41404150,and 11303049);Ministry of Science and Technology(Grant No.2011CB811403) 摘　　要：round-the-clock solar observations with full-disk coverage of vector magnetograms and multi-wavelength images demonstrate that solar active regions(ARs) are ultimately connected with magnetic field. Often two or more ARs are clustered, creating a favorable magnetic environment for the onset of coronal mass ejections(CMEs). In this work, we describe a new type of magnetic complex: cluster of solar ARs. An AR cluster is referred to as the close connection of two or more ARs which are located in nearly the same latitude and a narrow span of longitude. We illustrate three examples of AR clusters, each of which has two ARs connected and formed a common dome of magnetic flux system. They are clusters of NOAA(i.e., National Oceanic and Atmospheric Administration) ARs 11226 & 11227, 11429 & 11430, and 11525 & 11524. In these AR clusters, CME initiations were often tied to the instability of the magnetic structures connecting two partner ARs, in the form of inter-connecting loops and/or channeling filaments between the two ARs. We show the evidence that, at least, some of the flare/CMEs in an AR cluster are not a phenomenon of a single AR, but the result of magnetic interaction in the whole AR cluster. The observations shed new light on understanding the mechanism(s) of solar activity. Instead of the simple bipolar topology as suggested by the so-called standard flare model, a multi-bipolar magnetic topology is more common to host the violent solar activity in solar atmosphere. 关键词：日冕物质抛射太阳活动区原子团簇结构连接 ARS 观测矢量拓扑结构太阳大气

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Cluster of solar active regions and onset of coronal mass ejections

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