An advective solar-type dynamo without the α effect

Astronomy and Astrophysics

Volumn 508, Issue 1, 2009, Pages 9-16

  Seehafer, N ^a   Pipin, V V ^b  

^a UNIVERSITY OF POTSDAM   (Germany)

^b INSTITUTE OF SOLAR TERRESTRIAL PHYSICS   (Russian Federation)

Author keywords

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

Indexed keywords

AXISYMMETRIC; DIFFERENTIAL ROTATION; DYNAMO MODELS; EQUATORIAL PLANES; HALF CYCLE; HELIOSEISMIC; INHOMOGENEITIES; MEAN FIELD MODELS; MEAN-FIELD; MERIDIONAL CIRCULATION; MERIDIONAL FLOWS; MODEL CALCULATIONS; OSCILLATORY BEHAVIORS; RADIAL PROFILES; SHEAR-CURRENT EFFECTS; SOLAR MAGNETIC FIELDS; SOLAR OBSERVATIONS; STANDARD MODEL; STARS: MAGNETIC FIELD; TURBULENT CONVECTION; TURBULENT DYNAMO;

ELECTROMOTIVE FORCE; FLUID DYNAMICS; HEAT CONVECTION; INTERACTIVE DEVICES; MAGNETIC FIELDS; MAGNETIC MATERIALS; MAGNETOHYDRODYNAMICS; ROTATION; STARS; SUN;

DC GENERATORS;

EID: 71849111884     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912614     Document Type: Article

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