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Flare-Induced Coronal Disturbances Observed with Norikura 'NOGIS' Coronagraph: A CME Onset

机译:用Norikura“Nogis”orononagraph观察到眩光诱导的冠状动脉:CME发作

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We present the first detection of a CME onset in the coronal green line emission (Fe XIV 5303 ?, 2 MK) by a 2D Doppler coronagraph "NOGIS" at the Norikura Solar Observatory, NAOJ. Different from a typical CME that evolves within a single magnetic flux system with a single magnetic neutral line, NOGIS observed a CME that evolved across two neighboring magnetic flux systems; a flare-productive active region and an aggregate of face-on coronal loops with a streamer on its top. An early precursor of the event was a density enhancement of 2 MK plasma in the space between the two magnetic flux systems. In association with an M6.5 flare that occurred at the active region, a blueshifted upward jet and expansion appeared from a site where the legs of the two systems apparently connected each other. This expansion later evolved into a partial halo CME with an angular extent covering the latitudinal range of the two systems. These observational properties suggest the existence of a CME corridor that is consisted of neighboring multiple magnetic-flux systems through which a huge CME launches off.
机译:我们在Naoj的Norikura太阳天文台的2D多普勒·普通群“Nogis”介绍了在冠状绿线发射(Fe XIV 5303',2 MK)中的CME发作的第一次检测。不同于典型的CME,其在单个磁通系统中发展,具有单个磁性中性线,Nogis观察到跨两个相邻的磁通系统演变的CME;耀斑生产的有源区和顶部冠状环的聚集体,其顶部有飘带。事件的早期前体是两个磁通系统之间的空间中的2 Mk等离子体的密度增强。与在活动区域​​发生的M6.5的耀斑结合,从两种系统的腿显然彼此连接的位置出现了蓝色向上的向上射流和膨胀。这种展开稍后将覆盖两个系统的纬度范围的角度范围的部分光环CME。这些观察性质建议存在由邻近的多个磁通系统组成的CME走廊,通过该系统,巨大的CME推出。

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