论文标题
部分细丝爆发的多大波长度观察2011年6月13日
Multiwavelength observations of a partial filament eruption on 13 June 2011
论文作者
论文摘要
在本文中，我们报告了2011年6月13日在NOAA活动区域11236中与C1.2级别的部分细丝爆发的多波长度观察。该事件发生在大气成像组装（AIA）的东部肢体（AIA）的东部肢体（AIA），船上solar Dynameration（Solar Dynameration（Solar Dynameration）的固定式（SDO）固定在近距离（SDO），并在近距离范围内固定在固定位置（SDO），以至于固定在近距离范围。在太阳陆地关系天文台（立体声）航天器后面的成像仪（EUVI）。在喷发期间，细丝分为两个部分：主要部分和失控的部分。主要部分沿着封闭环路流动，并在循环顶部经历分叉。一些材料向前移动并到达远程脚尖，而另一些材料则返回原始脚尖。失控的部分沿开放式线路流动，这是由耀斑相关的III型无线电爆发证明的。失控的部分也发生分叉。逃脱电晕的上部分支以324 km S-1的速度演变成射流的狭窄冠状质量射血（CME），而下部分支则落回太阳表面。提出了示意图的动画片来解释事件，并提供了部分细丝爆发的新机制
In this paper, we report the multiwavelength observations of the partial filament eruption associated with a C1.2 class flare in NOAA active region 11236 on 13 June 2011. The event occurred at the eastern limb in the field of view (FOV) of Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) spacecraft and was close to the disk center in the FOV of Extreme-UltraViolet Imager (EUVI) on board the behind Solar Terrestrial Relations Observatory (STEREO) spacecraft. During eruption, the filament splits into two parts: the major part and runaway part. The major part flows along closed loops and experiences bifurcation at the loop top. Some of the materials move forward and reach the remote footpoint, while others return back to the original footpoint. The runaway part flows along open field lines, which is evidenced by a flare-related type III radio burst. The runaway part also undergoes bifurcation. The upper branch of escapes the corona and evolves into a jet-like narrow coronal mass ejection (CME) at a speed of 324 km s-1, while the lower branch falls back to the solar surface. A schematic cartoon is proposed to explain the event and provides a new mechanism of partial filament eruptions
