小规模的光纤喷发作为太阳冠状孔中的X射线喷射的驱动器
Alphonse C Sterling1, Ronald L Moore2, David A Falconer2
1NASA/Marshall Space Flight Center, Huntsville, Alabama 35812, USA.
Nature
|July 7, 2015
概括
太阳X射线喷射是由微型电丝喷发驱动的,挑战了既有的新兴流量模型. 这表明一个普遍的磁力过程是太阳喷发的基础,从喷射到巨大的冠状质量喷射.
科学领域:
- 太阳物理 太阳物理
- 等离子体天体物理学
- 磁动力学是一种磁动力学.
背景情况:
- 传统上,太阳X射线喷射是由涉及磁重新连接的新兴流模型解释的.
- 这个模型预测了喷气基的X射线亮度,这是由于新出现的封闭磁场与环境开放磁场之间的重新连接.
研究的目的:
- 为了研究太阳X射线喷射的形成机制.
- 用高分辨率观测来测试新兴流量模型的有效性.
- 了解磁再连接在喷气形成中的作用.
主要方法:
- 分析了高分辨率的X射线和极紫外线观测结果.
- 研究了在冠状孔中形成的20个随机选择的X射线喷射.
- 观察数据与新兴流量模型的预测进行了比较.
主要成果:
- 与新兴流量模型相反,在所有研究的喷气中观察到微型线材喷发驱动重新连接.
- X射线的亮度来自于喷发的微细丝的"腿"的重新连接,类似于太阳耀斑.
- 以前质疑该模型的发现是基于单喷气研究.
结论:
- 太阳X射线喷射是由微丝喷发驱动的,而不仅仅是由新兴流量模型驱动的.
- 磁性喷发是太阳大气中广泛运行的基本过程.
- 这种统一的观点有可能解释从小喷气到大太阳耀斑和冠状质量喷射等现象.
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