在太阳皇冠中的现场线滑动率
1School of Mathematics and Statistics, University of Glasgow, Glasgow, G12 8QQ UK.
概括
这项研究引入了太阳王冠中磁再连接的新局部描述,超越了非局部方法. 它将磁场线滑动与局部磁体几何联系起来,为这个基本过程提供了新的视角.
科学领域:
- * 太阳物理 太阳物理
- * 等离子体物理学
- * 天体物理学 * 天体物理学
背景情况:
- *磁再连接是太阳冠冕的一个关键动态过程.
- *目前研究重连接的方法主要是非局部的,依赖于全球磁拓.
- * 现有的理论,如通用磁再连接,也采用非局部措施.
研究的目的:
- * 介绍一篇关于磁再连接的新,本地描述.
- * 为了将场线滑动率与局部磁场几何联系起来.
- * 为了解太阳冠状的重新连接提供一个新的框架.
主要方法:
- * 开发了磁再连接的局部描述.
- * 用洛伦兹力和场对齐电流密度来描述局部磁体几何.
- * 应用了新方法对冠状磁场的分析和非线性无力模型.
主要成果:
- * 引入了场线滑动率的概念,作为重新连接的局部衡量标准.
- * 证明太阳冠冕中占主导地位的非理想项相当于异常电阻.
- * 显示了该方法的适应性,包括其他非理想的术语和一般化的欧姆定律.
结论:
- *本地描述补充了研究磁再连接的现有非本地方法.
- * 这一新框架为重新连接动态提供了更局部化的理解.
- * 该方法适用于各种冠状磁场配置,包括流动绳.
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