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Updated: Jul 12, 2026

Magnetically Induced Rotating Rayleigh-Taylor Instability
06:42

Magnetically Induced Rotating Rayleigh-Taylor Instability

Published on: March 3, 2017

在快速旋转的巨行星模型中,通过对流保持带状表面流

Z P Sun, G Schubert, G A Glatzmaier

    Science (New York, N.Y.)
    |April 30, 1993
    PubMed
    概括

    在旋转的流体中,热驱动的对流会产生带状区域流,模仿行星大气. 这些模拟支持对流作为木星和土星的原因.

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