太阳风的流和复杂性用排序多元分析 (ROMA) 进行了探测
Marius Echim1,2, Costel Munteanu2, Gabriel Voitcu2
1Royal Belgian Institute for Space Aeronomy, Avenue Circulaire 3, 1180 Bruxelles, Belgium.
Entropy (Basel, Switzerland)
|November 27, 2024
概括
排列顺序的多分形分析 (ROMA) 揭示了不同的太阳风流模式. 快速的太阳风表现出尺度依赖的波动,而缓慢的太阳风表现出完全发达的多分位动荡.
科学领域:
- 空间物理 空间物理
- 等离子体物理学的物理学
- 天体物理学 天体物理学
背景情况:
- 太阳风流是一种复杂的现象,对于理解太空中的能量传输至关重要.
- 在动荡等离子体中表征多分质性和尺度不变性对于天体物理学研究至关重要.
研究的目的:
- 应用排序式多分位分析 (ROMA) 来描述太阳风的流.
- 使用太空飞船数据,比较快速和缓慢的太阳风的多分质性质.
主要方法:
- 排序顺序的多分法分析 (ROMA) 用于分析波动.
- 使用范围有限的结构-功能分析来确定单碎指数.
- 分析了来自尤利西斯 (快速的太阳风) 和金星快递 (缓慢的太阳风) 飞船的数据.
主要成果:
- 快速的太阳风表现出规模依赖的波动:在动力尺度上持久,在惯性尺度上反持久.
- 缓慢的太阳风显示出完全发达的多分位动荡,在赫斯特指数的过渡中.
- 缓慢的太阳风中的小规模波动倾向于单碎形行为.
结论:
- 罗马有效地区分了快速和缓慢的太阳风流的多分法特征.
- 这些发现提供了关于太阳风动态的规模依赖性和复杂性的见解.
- 流结构的差异化对了解日球环境中的等离子体行为有影响.
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