A mechanism for differential rotation based on angular momentum transport by compressible convection

DOI10.1080/03091928708210111zbMath0635.76107OpenAlexW2031508999WikidataQ114640339 ScholiaQ114640339MaRDI QIDQ3775245

L. L. Kichatinov

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1080/03091928708210111

zbMATH Keywords

Reynolds equationcompressible convective motionsdensity-stratified rotating fluidIsorotational surfacesnon- diffusive fluxesquasi-isotropic convection

Mathematics Subject Classification ID

Reaction effects in flows (76V05) Diffusion and convection (76R99)

Cites Work

• Reynolds stresses and differential Rotation III. Zonal momentum fluxes in rapidly rotating stars
• Turbulent transport of angular momentum and differential rotation
• Reynolds stresses and differential rotation. I. On recent calculations of zonal fluxes in slowly rotating stars
• On the α-effect for slow and fast rotation
• Differential Rotation in Stars with Convective Envelopes.

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