Magnetoconvection and dynamo coefficients III. α-effect and magnetic pumping in the rapid rotation regime

Astronomy and Astrophysics

Volumn 455, Issue 2, 2006, Pages 401-412

  Kapyla P J ^a,b   Korpi, M J ^c   Ossendrijver, M ^b   Stix, M ^b  

^a UNIVERSITY OF OULU   (Finland)

^b KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^c UNIVERSITY OF HELSINKI   (Finland)

Author keywords

Convection; Magnetohydrodynamics (MHD); Stars: magnetic fields; Sun: magnetic fields; Turbulence

Indexed keywords

ATMOSPHERIC TURBULENCE; COMPUTATION THEORY; FORCE CONTROL; HEAT CONVECTION; MAGNETIC FIELD EFFECTS; OPTICAL PUMPING;

FIRST-ORDER SMOOTHING; MAGNETIC PUMPING; STARS: MAGNETIC FIELDS; SUN: MAGNETIC FIELDS;

MAGNETOHYDRODYNAMICS;

EID: 33748436388     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20064972     Document Type: Article

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