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

DOI10.1080/03091928008243659zbMath0454.76088OpenAlexW2167441660WikidataQ114640784 ScholiaQ114640784MaRDI QIDQ3902766

Günther Rüdiger

Publication date: 1980

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

Full work available at URL: https://doi.org/10.1080/03091928008243659

zbMATH Keywords

Reynolds stressesdifferential rotationstochastic motionszonal fluxes

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stochastic analysis (60H99)

Related Items (6)

Turbulent transport of angular momentum and differential rotation ⋮ A mechanism for differential rotation based on angular momentum transport by compressible convection ⋮ On the nature of the core-envelope boundary layer in a slowly rotating star ⋮ Reynolds stresses and differential Rotation III. Zonal momentum fluxes in rapidly rotating stars ⋮ Reynolds stresses and differential rotation II. Mean-field models ⋮ A model of the atmospheric convection zone with a large increase of rotation velocity between its bottom and top

Cites Work

• The nature of one mechanism of solar differential rotation
• Convective instability when the temperature gradient and rotation vector are oblique to gravity. I. Fluids without diffusion
• On the R<scp>EYNOLDS</scp> stresses in mean‐field hydrodynamics III. Two‐dimensional turbulence and the problem of differential rotation
• Differential Rotation in Stars with Convective Envelopes.
• On the thermal instability of a rotating-fluid sphere containing heat sources

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