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首页> 外文会议>COSPAR colloquium >MODELS OF ARCADE FLARES IN VIEW OF OBSERVATIONS BY YOHKOH, SOHO/EIT, AND TRACE
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MODELS OF ARCADE FLARES IN VIEW OF OBSERVATIONS BY YOHKOH, SOHO/EIT, AND TRACE

机译：展开型号的型号鉴于Yohkoh，SOHO / EIT和痕迹观察

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High-quality observations by Yohkoh, SOHO/EIT, and TRACE have indicated that arcade flares are energy release phenomena through magnetic reconnection. Our next interest is to clarify the global situation of the magnetic field in which the magnetic energy is stored and released. Such a global model should also explain the dark filament support and its eruption associated with arcade flares. In this paper, we briefly review global models proposed thus-far and discuss them in relation to some essential observational features. One of the promising global models is "quadruple magnetic source model", in which a dark filament with longitudinal magnetic field is supported in the current sheet between two magnetic loop systems and prevents magnetic reconnection. The results of MHD simulation based on this model show that the squeezing out of the dark filament allows reconnection of the two magnetic loop systems, and the relation between the dark filament eruption and the following arcade flare can be given natural explanation.
机译：Yohkoh，SOHO / EIT和痕迹的高质量观​​察表明，拱门耀斑通过磁重新连接是能量释放现象。我们的下一个兴趣是为了阐明磁能存储和释放磁场的全局情况。这种全球模型还应解释暗丝支撑及其与拱廊耀斑相关的喷发。在本文中，我们简要介绍了迄今为止建议的全球模型，并与一些基本的观察特征相关。承诺的全球模型之一是“四重磁源模型”，其中具有纵向磁场的暗灯丝在两个磁环系统之间的当前片中支撑在当前片中，并防止磁重新连接。基于该模型的MHD仿真结果表明，暗丝的挤出允许重新连接两个磁回路系统，并且可以给予自然的解释暗丝爆发与以下拱道闪光之间的关系。

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