Turbulent Mixing in Stars: Theoretical Hurdles-Reference-Cited by-同舟云学术

Turbulent Mixing in Stars: Theoretical Hurdles

Published:2009-08 Issue:S265 Volume:5 Page:106-110
ISSN:1743-9213
Container-title:Proceedings of the International Astronomical Union
language:en
Short-container-title:Proc. IAU

Author:

Arnett W. David,Meakin Casey

Abstract

AbstractA program is outlined, and first results described, in which fully three-dimensional, time dependent simulations of hydrodynamic turbulence are used as a basis for theoretical investigation of the physics of turbulence. The inadequacy of the treatment of turbulent convection as a diffusive process is indicated. A generalization to rotation and magnetohydrodynamics is indicated, as are connections to simulations of 3D stellar atmospheres.

Publisher

Cambridge University Press (CUP)

Subject

Astronomy and Astrophysics,Space and Planetary Science

Reference25 articles.

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3. CORONAE AS A CONSEQUENCE OF LARGE-SCALE MAGNETIC FIELDS IN TURBULENT ACCRETION DISKS

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