多源连接是太阳风在日球变化的驱动力
Stephanie L Yardley1,2,3,4, David H Brooks5, Raffaella D'Amicis6
1Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle Upon Tyne, UK.
概括
太阳轨道器的数据显示,太阳风的变化是由多个太阳能源的磁连接变化所驱动的. 这有助于理解复杂的日球结构和太阳风起源.
科学领域:
- 空间物理 空间物理
- 太阳物理 太阳物理
- 等离子体物理学的物理学
背景情况:
- 太阳风是来自太阳的带电粒子流,具有高度结构,来自冠状孔的快速流和缓慢流的争论来源.
- 了解太阳风的起源和复杂性对于日球物理学至关重要.
研究的目的:
- 为了确定太阳轨道器观察到的太阳风变化的来源.
- 了解日球复杂结构背后的驱动因素.
主要方法:
- 结合磁场建模和光谱技术.
- 利用太阳轨道器的高分辨率观测和现场测量.
- 分析了磁连接到太阳能源的时空变化.
主要成果:
- 太阳风在0.5天文单位的变化与连接不同太阳区域的磁场脚点的变化有关.
- 观察到从快速到Alfvénic的过渡到缓慢的太阳风,包括冠状质量喷射的破坏.
- 证明了连接从冠状孔边界移动到活动区域12961和12957.
结论:
- 太阳风的变化是由磁性连接到太阳大气中的多个来源的动态变化所驱动的.
- 这些发现通过将它们与特定的太阳能源区域联系起来来解释现场观测.
- 结果适用于理解地球附近观察到的太阳风现象.
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