Global MHD simulations of stratified and turbulent protoplanetary discs

Astronomy and Astrophysics

Volumn 496, Issue 3, 2009, Pages 597-608

  Fromang, S ^a,b   Nelson, R P ^c  

^a CEA SACLAY   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

Author keywords

Accretion, accretion disks; Magnetohydrodynamics (MHD); Methods: numerical; Turbulence

Indexed keywords

ACCRETION DISCS; ACCRETION, ACCRETION DISKS; DIFFUSION COEFFICIENTS; DUST DENSITY; DUST GRAINS; DUST PARTICLE; GLOBAL MHD SIMULATION; GRAVITATIONAL SETTLING; GRID-BASED; MAGNETIZED CORONA; MAGNETOHYDRODYNAMICS (MHD); MAGNETOROTATIONAL INSTABILITY; METHODS: NUMERICAL; MHD TURBULENCE; MOMENTUM TRANSPORTS; NUMERICAL SIMULATION; ORDERS OF MAGNITUDE; QUASI-STEADY STATE; SIMPLE MODEL; SIMULATION RESULT; SPATIAL DISTRIBUTION; STANDARD MODEL; TURBULENT DIFFUSION; TWO-FLUID; UPPER LAYER; VELOCITY FLUCTUATIONS; VERTICAL PROFILE; VERTICAL VELOCITY;

DIFFUSION; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; FLUID DYNAMICS; MAGNETOHYDRODYNAMICS; NUMERICAL METHODS; SIZE DISTRIBUTION; TURBULENCE;

SIMULATORS;

EID: 65949091787     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811220     Document Type: Article

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