Large-scale Vortices in Rapidly Rotating Rayleigh–Bénard Convection at Small Prandtl number

نویسندگان

چکیده

Abstract One prominent feature in the atmospheres of Jupiter and Saturn is appearance large-scale vortices (LSVs). However, mechanism that sustains these LSVs remains unclear. possible are driven by rotating convection. Here, we present numerical simulation results on a rapidly Rayleigh–Bénard convection at small Prandtl number Pr = 0.1 (close to turbulent numbers Saturn). We identified four flow regimes our simulation: multiple vortices, coexisting cyclone anticyclone, cyclone, turbulence. The formation requires two conditions be satisfied: vertical Reynolds large ( Re z ≥ 400 ), Rossby Ro ≤ 0.4). A first appears when decreases smaller than 0.4. When further 0.1, anticyclone emerges. have studied heat transfer result reveals more efficient anticyclonic region cyclonic region. Besides, find 2D effect increases 3D transporting convective flux as rotation rate increases. aspect ratio has an critical emergence LSVs. Our provide helpful insights into understanding dynamics gas giants.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2021

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac2c68