MRI-driven turbulent transport: The role of dissipation, channel modes and their parasites

Astronomy and Astrophysics

Volumn 516, Issue 18, 2010, Pages

  Longaretti, P Y ^a   Lesur, G ^b  

^a UNIV GRENOBLE ALPES   (France)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

accretion; accretion disks; magnetohydrodynamics (MHD); turbulence

Indexed keywords

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); MAGNETOHYDRODYNAMICS; PRANDTL NUMBER; REYNOLDS NUMBER; TURBULENCE;

ACCRETION; ACCRETION DISKS; AXISYMMETRIC; BOX SIZES; FLUID VISCOSITY; LINEAR MODES; MAGNETIC PRANDTL NUMBERS; MAGNETIC REYNOLDS NUMBER; NUMERICAL SIMULATION; PARASITIC MODE; POWER-LAW DEPENDENCES; QUASI-LINEAR; TURBULENT TRANSPORTS; UNSTABLE MODES;

TRANSPORT PROPERTIES;

EID: 77957834356     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014093     Document Type: Article

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