The Study of Ribbon Separation in a Two-ribbon Flare

XIE Wen-bin

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The Study of Ribbon Separation in a Two-ribbon Flare

更新时间：2026-07-10

- The Study of Ribbon Separation in a Two-ribbon Flare
- Vol. 15, Issue 6, Pages: 82-85(2010)
- 作者机构：
  
  吉林师范大学教育技术与传播学院
- 作者简介：
- 基金信息：
- DOI：
  CLC： P182.52
- Published：2010
- 稿件说明：
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XIE Wen-bin. The Study of Ribbon Separation in a Two-ribbon Flare[J]. 2010, 15(6): 82-85.
DOI：

XIE Wen-bin. The Study of Ribbon Separation in a Two-ribbon Flare[J]. 2010, 15(6): 82-85. DOI：

摘要

太阳耀斑是最剧烈的太阳活动现象

耀斑最普遍的观测现象是耀斑带向磁中性线两侧分离.通过一个典型的太阳双带耀斑事件研究耀斑带分离运动的规律.研究发现:耀斑带的分离速度和纵向磁场是负相关的;从爆发时间上看

这种相关在耀斑峰值的时候最弱;耀斑爆发过程中

最强的重联发生在硬X射线辐射源区域.此外

在耀斑爆发期间

磁重联率和耀斑带的分离速度有相似的变化趋势.

Abstract

Solar flare is one of the most prominent manifestations of solar eruptions.The often-observed ribbon expansion is the prevalent phenomena of the solar flare.In this paper

a study about the correlation between the speed of flare ribbon separation and the magnetic field is presented.A weak negative correlation is found between the ribbon separation speed and the longitudinal magnetic field.This correlation is the weakest around the peak of the flare.The strongest reconnection occurs at the position of the HXR...

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