在部分电离的太阳平稳态等离子体中存在阿尔夫文波
Nada F Alshehri1,2, Istvan Ballai1, Gary Verth1
1Plasma Dynamics Group, School of Mathematical and Physical Sciences, The University of Sheffield, Hicks Building, Hounsfield Road, Sheffield, S3 7RH UK.
概括
稳定流动显著改变了部分电离的太阳等离子体中的阿尔弗温波,影响了它们的传播,缩,甚至导致了由于离子中性碰撞的新波模式.
科学领域:
- 等离子体物理学的物理学
- 太阳物理 太阳物理
- 天体物理学 天体物理学
背景情况:
- 阿尔夫恩波对于太阳等离子体中的能量传输至关重要.
- 部分电离和离子中性碰撞在太阳大气中很常见.
- 背景流可以显著影响波动力学.
研究的目的:
- 在具有稳定流动的部分电离太阳等离子体中研究阿尔弗文波特性.
- 了解流动和离子中性碰撞如何改变波浪的传播和阻尼.
- 探索由这些条件引起的新波现象.
主要方法:
- 采用了两流体模型,将离子和中性处理为单独的碰撞流体.
- 集成的背景稳定流动为充电和中性粒子.
- 使用分析分散分析和数值解决方案.
主要成果:
- 稳定的流动会对阿尔夫恩波的特性造成实质性修改.
- 观察到多普勒转移,传播方向逆转和流量依赖的减压率.
- 确定了一种与中性流和碰撞合以及流动驱动模式转换相关的新波形态.
结论:
- 稳定的流动和离子中性碰撞在太阳大气中的阿尔弗温波行为中起着关键作用.
- 这些相互作用导致复杂的波动,包括模式转换.
- 这些发现为能源运输和部分电离太阳区域的现象提供了新的见解.
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