皮科弗莱尔喷射驱动太阳风从太阳的冠状孔中涌出
L P Chitta1, A N Zhukov2,3, D Berghmans2
1Max-Planck-Institut für Sonnensystemforschung, 37077 Göttingen, Germany.
概括
从太阳冠孔喷出的小规模喷气可能是太阳风的来源. 这些由太阳轨道探测器观测到的小火焰喷射提供高温等离子体,
科学领域:
- 太阳物理
- 血物理
- 天体物理学
背景情况:
- 冠状孔是太阳上的开放磁场线的区域.
- 它们是已知的太阳风来源,
研究的目的:
- 调查在冠状孔内产生太阳风的小规模过程.
- 了解这些区域如何产生高温等离子体.
主要方法:
- 使用太阳轨道飞船的极紫外线成像器观测冠状孔.
- 小规模喷气事件的识别和分析.
主要成果:
- 标识了几百公里的间歇喷气,持续20-100秒,速度约为100公里/秒.
- 这些喷气是由磁性重新连接提供动力, 并拥有Picoflare动能.
- 这些喷气被发现在观察到的冠状孔内广泛存在.
结论:
- 它们是维持太阳风所需的高温等离子体的可信来源.
- 太阳风很可能从冠状孔中以小规模的间歇性流出.
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