在太阳突出处的磁热对流
Thomas Berger1, Paola Testa, Andrew Hillier
1Lockheed Martin Advanced Technology Center, Solar and Astrophysics Laboratory, O/ADBS B/252, 3251 Hanover Street, Palo Alto, California 94304, USA. berger@lmsal.com
Nature
|April 15, 2011
概括
太阳冠状腔内的更热的等离子泡提供浮力,导致雷利-泰勒不稳定性. 这揭示了太阳大气层中一种新的磁热对流机制,解释了冠状体质量弹射演变.
科学领域:
- 太阳物理 太阳物理
- 血物理学的等离子体物理学
- 天体物理学 天体物理学
背景情况:
- 冠状腔是太阳大气中较大,密度较低的区域,由磁流绳组成.
- 这些空洞进化,并可以作为冠状质量喷射爆发,影响行星磁层.
- 冠状腔的进化机制仍然不太了解.
研究的目的:
- 为了研究在冠状腔中的极冠突出区域内等离子体泡的性质和浮力.
- 阐明这些气泡在冠状腔向喷发的进化中的作用.
- 挑战和完善当前关于太阳突出和冠状腔的水磁概念.
主要方法:
- 极冠突出点的同时光学和极紫外线 (EUV) 观测.
- 在观察到的"泡"和覆盖突出物质中的血温度分析.
- 在观察到的等离子体特性背景下研究雷利-泰勒不稳定性.
主要成果:
- 在极冠突出部内观察到的气泡含有比周围突出部 (2.5-12 × 10^5 K) 显著更热的等离子体.
- 这种温度差异为气泡提供了浮力来源.
- 这些发现支持雷利-泰勒不稳定机制在冠状腔内形成羽毛.
结论:
- 冠状腔突出系统表现出一种新的磁热对流形式.
- 更热,浮动的等离子泡是了解冠状腔进化和喷发的关键.
- 这项研究挑战了现有的太阳突起和冠状腔的水磁模型.
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