A further uncertainty in the mixing length theory of convection in the structure of late-type stars

DOI10.1093/MNRAS/220.4.793zbMath0593.76089OpenAlexW2030996246MaRDI QIDQ3724003

Roger Tayler

Publication date: 1986

Published in: Monthly Notices of the Royal Astronomical Society (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1093/mnras/220.4.793

zbMATH Keywords

energy transportconvective fluxsurface magnetic fieldsconvection in starslate-type main-sequence starmixing length theory of convectionratio of the mixing length to the pressure scale height

Mathematics Subject Classification ID

Hydrology, hydrography, oceanography (86A05) General theory of rotating fluids (76U05) Diffusion and convection (76Rxx)

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