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Updated: Jul 2, 2025

Magnetically Induced Rotating Rayleigh-Taylor Instability
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螺旋式动力马的增长和和在适度与极端磁力雷诺兹数的适度和和

Hongzhe Zhou1, Eric G Blackman2

  • 1Tsung-Dao Lee Institute, Shanghai Jiao Tong University, 800 Dongchuan Road, Shanghai 200240, People's Republic of China and Nordita, KTH Royal Institute of Technology and Stockholm University, Hannes Alfvéns väg 12, SE-10691 Stockholm, Sweden.

Physical review. E
|February 17, 2024
PubMed
概括

在封闭体积中的天体物理磁场增长显示了一个预和状态,其中增长率独立于磁力雷诺兹数 (Rm). 这一发现为恒星和星系的闭 dynamo 模型带来了新的乐观.

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