TURBULENCE IN ASTROPHYSICS: Stars

▪ Abstract Turbulence is ubiquitous in astrophysics, ranging from cosmology, interstellar medium to stars, supernovae, accretion disks, etc. Large scales and small viscosities combine to form large Reynolds numbers. Because it is not possible in a single article to review all the above scenarios, w...

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Bibliographic Details
Published in:	Annual review of fluid mechanics Vol. 30; no. 1; pp. 167 - 198
Main Authors:	Canuto, V. M., Christensen-Dalsgaard, J.
Format:	Journal Article
Language:	English
Published:	Palo Alto, CA Annual Reviews 01.01.1998 Annual Reviews, Inc
Subjects:	Astronomy Earth, ocean, space Exact sciences and technology Stars Stellar characteristics and properties Stellar structure, interiors, evolution, nucleosynthesis, ages Differential rotation Astroseismology Turbulence Stars Theoretical study Turbulent convection Star models Convective overshooting Reynolds stress Helioseismology Closure model Radiative properties Stellar interiors
ISSN:	0066-4189, 1545-4479
Online Access:	Get full text
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