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Signatures of Magnetic Reconnection in Solar Eruptive Flares: A Multi-wavelength Perspective

机译:太阳爆发耀斑中磁重联的特征:多波长视角

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In this article, we review some key aspects of a multi-wavelength flare which have essentially contributed to form a standard flare model based on the magnetic reconnection. The emphasis is given on the recent observations taken by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) on the X-ray emission originating from different regions of the coronal loops. We also briefly summarize those observations which do not seem to accommodate within the canonical flare picture and discuss the challenges for future investigations.
机译:在本文中,我们回顾了多波长耀斑的一些关键方面,它们在基于磁重连的基础上形成了标准的耀斑模型方面做出了重要贡献。重点是鲁汶拉玛特高能太阳光谱成像仪(RHESSI)对源自冠状loop不同区域的X射线发射所进行的近期观测。我们还简要总结了那些似乎不适合常规耀斑图像的观察,并讨论了未来研究的挑战。

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