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XRT and EIS Observations of Reconnection Associated Phenomena

机译：XRT和EIS的重组相关现象的观察

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Based on the results of numerical simulations, we sythesized EIS and XRT images of reconnection flows associated with an eruptive flare. The results suggest that reconnection inflows can be observed as pairs of blue- and red-shifted components just above the X-ray arcade in the low temperature lines. It is found that the Doppler velocities are larger in the lower temperature line spectra. Reconnection outflows can also be observed as pairs of blue- and redshifted components with an asymmetry in the high temperature line spectra.

机译：基于数值模拟的结果，我们将EIS和XRT图像的重组流与爆发耀斑相关联。结果表明，重新连接流入可以被观察为刚刚在低温线上的X射线拱廊上方的蓝色和红色移位组件对。发现多普勒速度在较低温度线光谱中较大。还可以观察到重组外流作为具有高温线谱中不对称的蓝色和红移组分的对。

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《Solar-B Science Meeting》|2007年||共6页
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作者
Daikou Shiota; Hiroaki Isobe; David H. Brooks; Peng-Fei Chen; Kazunari Shibata;
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原文格式 PDF
正文语种
中图分类太阳物理学;
关键词
XRT; EIS; Phenomena;

机译：Chem;在？;

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4. XRT and EIS Observations of Reconnection Associated Phenomena [C] . Daikou Shiota, Hiroaki Isobe, David H. Brooks, Solar-B Science Meeting . 2007

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XRT and EIS Observations of Reconnection Associated Phenomena

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