南方高速流:来自乌利塞斯号上的SWICS仪器的结果
J Geiss1, G Gloeckler, R von Steiger
1Physikalisches Institut, University of Bern, Switzerland.
概括
来自南方冠状孔的高速太阳风稳定且有限. 电子温度达到150万克尔文,这表明需要额外的动量来加速北极风.
科学领域:
- 太阳物理 太阳物理
- 血物理学的等离子体物理学
- 太空物理学 太空物理学
背景情况:
- 太阳风是从太阳的上层大气层释放出来的带电粒子的流,称为冠状.
- 冠状孔是太阳大气层中磁场线开放的区域,允许太阳风逃逸.
研究的目的:
- 为了分析来自南方冠状孔的高速太阳风的特征.
- 为了确定冠状孔内的电子温度和元素组成.
- 为了研究极地风的加速机制.
主要方法:
- 来自南方冠状孔的高速太阳风数据的分析.
- 使用电荷状态测量推断电子温度.
- 检查重元素丰富度以了解血成分.
主要成果:
- 太阳风流非常均,稳定,并且有明显的界限,延伸到冠冕和染色体.
- 冠状孔内的电子温度在3个太阳半径内达到大约150万凯尔文.
- 没有观察到重元素的显著耗尽.
结论:
- 太阳风和等离子体组成的观测特性表明,标准加速模型可能不足.
- 很可能需要一个额外的动量源来解释极地风的加速.
- 需要进一步的研究才能充分理解极地太阳风的动态和加速过程.
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