Diffusion coefficient of a passive contaminant in a local MHD model of a turbulent accretion disc

Monthly Notices of the Royal Astronomical Society

Volumn 358, Issue 3, 2005, Pages 1055-1060

  Carballido, Augusto ^a,b   Stone, James M ^b   Pringle, James E ^a  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b PRINCETON UNIVERSITY   (United States)

Author keywords

Accretion, accretion discs; MHD

Indexed keywords

CONTAMINATION; DIFFUSION; IMPURITIES; MAGNETOHYDRODYNAMICS; PRANDTL NUMBER;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; CONTINUITY EQUATIONS; FUNCTION OF TIME; MAGNETOHYDRODYNAMIC MODEL; MAGNETOROTATIONAL INSTABILITY; MASS-FRACTION; NUMERICAL MAGNETOHYDRODYNAMIC SIMULATION; RADIAL DIFFUSION; RADIAL PROFILES;

SHEAR STRESS;

EID: 17444362673     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.08850.x     Document Type: Article

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