磁和绳索作为太阳爆发的关键
Tahar Amari1, Aurélien Canou2, Jean-Jacques Aly3
1CPHT, Ecole Polytechnique, CNRS, Université Paris-Saclay, Route de Saclay, 91128 Palaiseau, France.
Nature
|February 9, 2018
概括
限制太阳耀斑是由扭曲的磁流绳的不稳定引起的, 不仅仅是复杂的磁拓. 这条流动绳
科学领域:
- 太阳物理
- 等离子天体物理学
- 磁动力学
背景情况:
- 太阳耀斑是被归类为爆发或封闭的能量冠状事件.
- 封闭式耀斑缺乏冠状质量喷射, 它们的触发机制仍在争论中.
- 之前的模型集中在磁形拓或流绳不稳定性上, 缺乏确切的观测证据.
研究的目的:
- 通过详细的磁场建模来研究太阳耀斑的触发机制.
- 区分拓复杂性和流绳不稳定性作为主要原因.
- 用测量的光球磁场作为静态和动态模型的输入.
主要方法:
- 使用静态模型模拟爆发前的冠状磁性状态.
- 使用动态模型捕捉爆发事件中的演变.
- 集成测量光球磁场数据作为模型的输入.
主要成果:
- 在整个事件中,磁流绳是必不可少的,以匹配观察数据.
- 流线的发展缓慢,和, 然后由于扭曲的不稳定性爆发.
- 限制磁场阻止了更大的喷发, 但它的弱点影响了事件的能量.
结论:
- 封闭式火焰主要是由扭曲的磁流绳的不稳定性驱动的.
- 磁拓影响X射线发射局部化,但不是主要的触发因素.
- 封闭磁场的强度决定了火焰是否会被封闭,或者是否会成为具有冠状质量喷射的爆发事件.
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