A model of thermal convection in the major planets with a strongly density-stratified atmospheric layer

DOI10.1080/03091928508245433zbMath0585.76126OpenAlexW2074307929WikidataQ114640439 ScholiaQ114640439MaRDI QIDQ3710276

Jun-Ichi Yano

Publication date: 1985

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091928508245433

zbMATH Keywords

convective instabilityatmospheric layer of major planetsexpansion parametersself-gravitating rotating spherical fluidspherical Boussinesq fluidtwo-layer model of thermal convection

Mathematics Subject Classification ID

Absolute and convective instability and stability in hydrodynamic stability (76E15) General theory of rotating fluids (76U05) Reaction effects in flows (76V05) Galactic and stellar dynamics (85A05) Forced convection (76R05)

Cites Work

• A model of mean zonal flows in the major planets
• On the Finite amplitude thermal instability of a rapidly rotating fluid sphere
• On the thermal instability of a rotating-fluid sphere containing heat sources
• Thermal instabilities in rapidly rotating systems

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