Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations

Astronomy and Astrophysics

Volumn 411, Issue 3, 2003, Pages 321-327

  Yousef, T A ^a   Brandenburg, A ^b   Rudiger G ^c  

^a NORWEGIAN UNIVERSITY OF SCIENCE AND TECHNOLOGY   (Norway)

^b NORDITA   (Denmark)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Magnetohydrodynamics (MHD); Turbulence

Indexed keywords

APPROXIMATION THEORY; DIFFUSION; KINEMATICS; KINETIC ENERGY; MAGNETOHYDRODYNAMICS; MICROSCOPIC EXAMINATION; PRANDTL NUMBER; QUENCHING; REYNOLDS NUMBER; TURBULENCE; VISCOSITY;

HELICAL MEAN FIELDS; MAGNETOROTATIONAL INSTABILITY;

ASTROPHYSICS;

EID: 0344944237     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031371     Document Type: Article

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