在冠状循环中滑动磁再连接.
Guillaume Aulanier1, Leon Golub, Edward E Deluca
1Observatoire de Paris, Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie (UPMC), Université Paris Diderot, 92190 Meudon, France. guillaume.aulanier@obspm.fr
概括
太阳耀斑是由磁再连接引起的. 新证据表明,一个滑动磁再连接过程,其中磁场线滑过彼此,是理解太阳耀斑和冠状热的关键.
科学领域:
- 血物理学的等离子体物理学
- 太阳物理 太阳物理
- 天体物理学 天体物理学
背景情况:
- 太阳冠状循环中的磁再连接驱动太阳耀斑和冠状加热.
- 标准模型假设在不连续的磁场映射中瞬间磁场线断裂.
- 另一个滑动磁再连接模式可能发生在连续但的场度梯度.
研究的目的:
- 为了调查太阳冠冕磁再连接滑落的存在和影响.
- 为滑动磁再连接模型提供观察支持.
- 为解释太阳能和实验室等离子体中的磁再连接提供信息.
主要方法:
- 来自Hinode航天器的软X射线观测的分析.
- 对冠状环的快速双向运动的观察.
- 观察到的现象与磁再连接的理论模型进行比较.
主要成果:
- 观察到的冠状环的快速双向运动提供了滑动磁重连接的证据.
- 这种模式在磁场映射是连续的,但有的梯度的地方运行.
- 支持标准即时重新连接模型的替代方案.
结论:
- 滑动磁再连接是太阳冠冕中一个可行的过程.
- 在研究太阳耀斑和冠状热时,应该考虑这种机制.
- 这些发现对于太阳能和实验室等离子体重新连接研究都很重要.
相关概念视频
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