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Updated: Jun 17, 2025

Magnetically Induced Rotating Rayleigh-Taylor Instability
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双等离子体中的无碰撞磁旋动荡:稳态动力学,粒子加速和辐射冷却

Fabio Bacchini1,2, Vladimir Zhdankin3,4, Evgeny A Gorbunov1

  • 1Centre for Mathematical Plasma Astrophysics, Department of Mathematics, <a href="https://ror.org/05f950310">KU Leuven</a>, Celestijnenlaan 200B, B-3001 Leuven, Belgium.

Physical review letters
|August 9, 2024
PubMed
概括

这项研究使用3D模拟演示了动力磁旋动流动中的非热粒子加速. 它揭示了在动力尺度上升的流光谱和角度动量传输.

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