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

DOI10.1080/03091928608210088zbMath0644.76051OpenAlexW2016958070WikidataQ114640402 ScholiaQ114640402MaRDI QIDQ3787667

Jean-Louis Tassoul, Monique Tassoul

Publication date: 1986

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

Full work available at URL: https://doi.org/10.1080/03091928608210088

zbMATH Keywords

differential rotationlarge-scale motionslarge-scale meridional currentssingle, nonmagnetic, early-type starsmall-scale baroclinic eddies

Mathematics Subject Classification ID

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

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Cites Work

• The nature of one mechanism of solar differential rotation
• Proposal of a new method of solution of the unsteady non-linear eddington–vogt–sweet circulation
• Reynolds stresses and differential rotation. I. On recent calculations of zonal fluxes in slowly rotating stars

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