相关实验视频
Updated: Jul 19, 2025

06:42
Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
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在乱无碰撞等离子体中产生近等分磁场
Lorenzo Sironi1, Luca Comisso1, Ryan Golant1
1Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027, USA.
Physical review letters
|August 18, 2023
概括
宇宙流可以在等离子体中产生和放大磁场. 模拟显示磁场呈指数增长和和,通过重新连接平衡,可能解释大规模的宇宙磁场.
科学领域:
- 天体物理学 天体物理学
- 等离子体物理学的物理学
- 宇宙磁力宇宙磁力宇宙磁力
背景情况:
- 宇宙中的磁场的起源和放大并未得到充分理解.
- 天体物理等离子体往往是动荡的,最初没有磁化.
研究的目的:
- 为了研究通过韦贝尔不稳定性的磁场产生.
- 为了研究磁场通过动态流程在乱等离子体中的放大磁场.
主要方法:
- 使用完全动态的粒子在细胞模拟.
- 模拟乱的,最初没有磁化的等离子体.
主要成果:
- 在动力动力发电机阶段观察到磁场强度的指数增长 (γB 0.4urms/L).
- 磁场能量和时大约是流运动能量的一半.
- 通过磁再连接的消散,用等离子体链表示,在和时平衡增长.
结论:
- 流可以有效地磁化无碰撞等离子体.
- 这一过程可以产生大规模,近等分的磁场,与星系和星系团有关.
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