Do eddington–sweet circulations exist?

DOI10.1080/03091928108243683zbMath0471.76111OpenAlexW1989739365WikidataQ114640733 ScholiaQ114640733MaRDI QIDQ3926292

Friedrich H. Busse

Publication date: 1981

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

Full work available at URL: https://doi.org/10.1080/03091928108243683

zbMATH Keywords

rotating baroclinic stararbitrary axisymmetric initial conditionsEddington-Sweet circulationsinternal-inertial modespurely zonal velocity fieldsteady meridional circulations do not exist

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (4)

Baroclinically-driven flows and dynamo action in rotating spherical fluid shells ⋮ Nonlinear diffusive instabilities in differentially rotating stars ⋮ An algorithm for computing the 2D structure of fast rotating stars ⋮ Hydromagnetic stability of a rotating baroclinic star

Cites Work

• Unnamed Item
• On Stellar Rotation: I. The Rotation of Upper Main-Sequence Stars
• The Importance of Rotation in Stellar Evolution

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