Reynolds stresses and differential Rotation III. Zonal momentum fluxes in rapidly rotating stars

DOI10.1080/03091928308210118zbMath0544.76124OpenAlexW2138077329WikidataQ114640591 ScholiaQ114640591MaRDI QIDQ3335387

Günther Rüdiger

Publication date: 1983

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

Full work available at URL: https://doi.org/10.1080/03091928308210118

zbMATH Keywords

sunequatorial accelerationinfluence of the Coriolis force on given turbulence modelsmodes of the non-diffusive zonal momentum fluxes (NDZF)non-trivial expansion of the NDZFprofiles for the angular velocity and horizontal Reynolds stressradial superrotation

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Planetary atmospheres (85A20)

Related Items (1)

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

Cites Work

• Reynolds stresses and differential rotation. I. On recent calculations of zonal fluxes in slowly rotating stars
• Reynolds stresses and differential rotation II. Mean-field models

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