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一个动态的磁张力导致了太阳爆发的失败
Clayton E Myers1,2, Masaaki Yamada2, Hantao Ji1,2,3
1Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA.
Nature
|December 25, 2015
概括
由于强烈的导向磁场, 太阳流绳可能无法爆发, 这造成了目前模型中缺失的张力. 这一发现解释了以前无法解释的
科学领域:
- 太阳物理
- 血物理
- 天体物理学
背景情况:
- 冠状质量喷射 (CMEs) 源自太阳的冠状.
- 磁流绳可以储存CME的能量.
- 体的不稳定性是流绳喷发的推测驱动因素.
研究的目的:
- 调查为什么体不稳定的流动绳有时无法爆发.
- 确定失败喷发背后的物理机制.
- 解决理论和观察之间的矛盾.
主要方法:
- 实验室实验模拟太阳磁现象.
- 在不同磁场条件下分析流绳动力学.
- 将实验结果与现有理论模型进行比较.
主要成果:
- 一个以前未知的喷发标准被确定.
- 强大的导向磁场防止流绳扭曲, 停止喷发.
- 观察到一个动态的状场张力, 停止喷发.
- 这种力量在目前的喷发模型中不存在.
结论:
- 导向磁场在防止扭曲的作用对于失败的喷发至关重要.
- 现有的模型无法解释状张力,限制了预测能力.
- 为了准确的CME预测,需要采用新的模型.
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