A model of the atmospheric convection zone with a large increase of rotation velocity between its bottom and top

DOI10.1007/BF00648543zbMath0543.76060OpenAlexW2139984412MaRDI QIDQ796383

Yu. V. Vandakurov

Publication date: 1982

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00648543

zbMATH Keywords

differential rotationfast rotationnonlinear azimuthal forceonly growing convective perturbationsslowly rotating stellar or planetary atmospheric convection zoneupper atmosphere of Venus

Mathematics Subject Classification ID

Planetary atmospheres (85A20) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Reynolds stresses and differential rotation. I. On recent calculations of zonal fluxes in slowly rotating stars

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