The penetration of meridional flow into the tachocline and its meaning for the solar dynamo

Astronomy and Astrophysics

Volumn 444, Issue 3, 2005, Pages

  Rudiger G ^a   Kitchatinov, L L ^a,b   Arlt, R ^a  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b INSTITUTE OF SOLAR TERRESTRIAL PHYSICS   (Russian Federation)

Author keywords

Hydrodynamics; Stars: interiors; Sun: interior

Indexed keywords

ASTROPHYSICS; HEAT CONVECTION; HYDRODYNAMICS; MAGNETIC FIELDS; SOLAR RADIATION;

CONVECTION ZONE; HARTMANN LAYER; STARS: INTERIORS; SUN: INTERIOR;

SOLAR SYSTEM;

EID: 29444431925     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200500209     Document Type: Article

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