在对离子中立漂移的两极扩散配方上,在不可忽视的漂移速度极限中漂移
1Department of Mathematics and Statistics, University of Exeter, Exeter EX4 4QF, UK.
概括
这项研究修改了部分电离等离体的两极扩散近似. 它表明,放松速度约束导致太阳大气模拟中的磁场扩散和摩擦加热减少.
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
- 太阳大气层动态 太阳大气层动态
背景情况:
- 两极扩散近似模型部分电离化等离子体动力学.
- 标准的双极扩散需要相比热速度的小漂移速度,以避免不可忽视的物种间碰撞.
研究的目的:
- 探索放松双极扩散中小漂移速度假设的后果.
- 为了制定一个新的感应方程,适用于更大的漂移速度.
- 为了研究对磁场扩散和摩擦加热的影响.
主要方法:
- 在没有小漂移速度约束的情况下开发了一个新的感应方程.
- 分析了大漂移速度极限及其对碰撞频率的影响.
- 将新配方应用于太阳染色体中的流体出现模拟.
主要成果:
- 制定了一个新的感应方程,将其缩小为小漂移速度的标准形式.
- 在大漂移速度极限中,磁场扩散比标准两极扩散减少.
- 摩擦加热由于磁场扩散的减少而减少.
- 模拟太阳流的出现显示了预测漂移速度的明显减少.
结论:
- 修订后的双极扩散模型为具有显著漂移速度的场景提供了更准确的描述.
- 这种改进的模型对理解部分电离等离子体中的能量传输和加热机制,特别是太阳大气中的能量传输和加热机制有影响.
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