无碰撞的近中性太阳风电流表模型
Sophie Boswell1, Thomas Neukirch1, Anton Artemyev2
1School of Mathematics and Statistics, University of St. Andrews, St. Andrews, UK.
概括
太阳风电流表表显示不对称的密度和温度变化. 一个具有修改电子分布函数的新模型揭示了这些等离子板内的亚结构.
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:
- 在现场太阳风测量显示了动力尺度电流板.
- 这些板通常是无力,具有一等级的血β.
- 观察到的粒子密度和温度不对称性在电流板上以前被建模.
研究的目的:
- 修改现有的无力无碰撞电流板模型.
- 仅仅是为了研究电子分布函数中一个额外项的影响.
- 分析得到的等离子体密度和电场子结构.
主要方法:
- 修改自相一致的无力无碰撞电流板模型.
- 在电子分布函数中包含一个额外的项,保持离子Maxwellian.
- 非线性近中性条件的数值解与安培尔定律并行.
主要成果:
- 磁场保持大约没有力.
- 一个非零的准中性电场出现.
- 在当前表中观察到额外的等离子体密度空间子结构.
结论:
- 修改后的模型提供了对当前表格动态的洞察力.
- 理论发现可能与观察到的当前板子结构有关.
- 不对称的电子分布可以在太阳风电流板中创建密度子结构.
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