On the validity of quasi-linear kinematic mean-field electrodynamics in astrophysical flows

Monthly Notices of the Royal Astronomical Society

Volumn 296, Issue 2, 1998, Pages 245-252

  Petrovay, K ^a   Zsargo J ^b  

^a INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^b UNIVERSITY OF TOLEDO   (United States)

Author keywords

Convection; Magnetic fields; MHD; Sun: interior

Indexed keywords

ASTROPHYSICS; KINEMATICS; MEAN FIELD THEORY; QUENCHING; TURBULENCE;

ASTROPHYSICAL FLOWS; CONVECTION; LINEAR APPROXIMATIONS; LINEAR KINEMATICS; MAGNETIC-FIELD; MEAN-FIELD; MEAN-FIELD THEORIES; QUASI-LINEAR; SUN: INTERIOR; WEAK MAGNETIC FIELDS;

MAGNETOHYDRODYNAMICS;

EID: 0006338113     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01231.x     Document Type: Article

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