Proposal of a new method of solution of the unsteady non-linear eddington–vogt–sweet circulation

DOI10.1080/03091928608210087zbMath0649.76021OpenAlexW2078185714WikidataQ114640403 ScholiaQ114640403MaRDI QIDQ3795391

Takeo Sakurai

Publication date: 1986

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

Full work available at URL: https://doi.org/10.1080/03091928608210087

zbMATH Keywords

unsteady nonlinear Eddington-Vogt-Sweet circulation

Mathematics Subject Classification ID

Turbulence (76F99) Galactic and stellar dynamics (85A05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

On the nature of the core-envelope boundary layer in a slowly rotating star

Cites Work

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• On almost rigid rotations. Part 2
• Spin-up of a strongly stratified fluid in a sphere
• The Importance of Rotation in Stellar Evolution
• Rotation and Stellar Evolution

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