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Updated: Jul 11, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
06:42

Magnetically Induced Rotating Rayleigh-Taylor Instability

Published on: March 3, 2017

在行星流中出现的异型和连贯结构.

J C McWilliams, J B Weiss, I Yavneh

    Science (New York, N.Y.)
    |April 15, 1994
    PubMed
    概括

    高分辨率的流体动力学模拟挑战同otropy的预测. 相反,行星规模的流动自我组织成连贯的,导致一个不动荡的状态.

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