在亚阿尔夫尼克太阳风中的随机加热
Trevor A Bowen1, Tamar Ervin1,2, Alfred Mallet1
1University of California, Space Sciences Laboratory, Berkeley, California 94720-7450, USA.
Physical review letters
|January 20, 2026
概括
无碰撞的等离子流动加热太阳风离子通过随机加热,而不是循环波. 这种间歇性加热机制与突破质子磁矩有关,对于理解太空和实验室等离子体中的能量转移至关重要.
科学领域:
- 血物理学的等离子体物理学
- 天体物理学 天体物理学
- 太空物理空间物理学
背景情况:
- 无碰撞流散是等离子体加热和运输的关键.
- 了解太阳风在太阳附近的加热对于太空天气和冠状物理学至关重要.
研究的目的:
- 为了分析帕克太阳探测器对亚阿尔夫尼克太阳风的观测.
- 确定该地区无碰撞流加热的主要机制.
主要方法:
- 在现场分析帕克太阳探测器数据.
- 研究波粒子相互作用和能量传递过程.
主要成果:
- 循环电子波的线性共振加热并不能解释观察到的离子能量化.
- 随机加热是由罕见的大幅度事件驱动的,解释了离子加热.
- 动荡的间歇性和质子磁矩的断裂被确定为关键因素.
结论:
- 随机加热是间歇性太阳风加热的主要机制.
- 这一发现对了解太阳冠状,天体物理等离子体和实验室环境中的流消散有意义.
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