日边离子层中的东向过渡. 封闭场线上的电动力学
Magnus F Ivarsen1, Jean-Pierre St-Maurice1, Glenn C Hussey1
1University of Saskatchewan, Department of Physics and Engineering Physics, Saskatoon, Saskatchewan, Canada.
Physical review. E
|November 18, 2025
概括
动荡的电流,以前认为白天很少见,在地球的白天离子层中观察到. 这些事件是由磁层等离子体波驱动的,挑战了关于太阳风与离子层相互作用的先前假设.
科学领域:
- 空间物理 空间物理
- 大气科学 大气科学
- 等离子体物理学的物理学
背景情况:
- 充满活力的极光通常会在夜边的电离层中驱动动荡荡的电流.
- 由于太阳极端紫外线辐射,白天的电离层等离子体具有很高的导电性,这被认为可以抑制流.
- 动荡的电流被认为在日边高度的电离层中是罕见的.
研究的目的:
- 为了调查发生和驱动小规模的等离子体流在白天离子层的驱动器.
- 挑战普遍认为电流流在白天不存在的观念.
- 为了确定磁层现象和电离层流之间的因果关系.
主要方法:
- 在地磁风暴期间利用两个轨道卫星的数据.
- 使用电子流量和波粒子相互作用数据推断了尖端和扩散极光的位置.
- 在E区域分析了等离子体密度梯度和电场.
主要成果:
- 在封闭磁场线上的日边E区域观察到多产的小规模等离子体流.
- 识别了散射极光,产生不稳定的等离子体密度梯度和强大的电场.
- 在磁层赤道附近的合唱波活动和流电流之间建立了相关性.
结论:
- 磁层等离子体波最终可以在白天离子层中驱动小规模的流.
- 当条件压倒其导电性时,短暂的,动荡的电流可以在白天离子层中形成.
- 这一发现对理解日边离子层电动力学有重大意义.
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