Are the strengths of solar cycles determined by converging flows towards the activity belts?

Astronomy and Astrophysics

Volumn 548, Issue , 2012, Pages

  Cameron, R H ^a   Schussler M ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Sun: activity; Sun: dynamo; Sun: surface magnetism

Indexed keywords

INTERACTIVE DEVICES; MAGNETIC FLUX; MAGNETIC POLARITY;

ACTIVE REGIONS; AXIAL DIPOLE; CONVERGING FLOW; EMPIRICAL CORRELATIONS; FLUX INPUTS; MAGNETIC REGION; NEAR-SURFACE; POLAR FIELDS; SOLAR CYCLE; SOLAR DYNAMO; STRONG CORRELATION; SUN: ACTIVITY; SURFACE DISTRIBUTIONS; SURFACE FLUX; SURFACE MAGNETISM; TILT ANGLE;

ELECTRIC GENERATORS;

EID: 84870032211     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219914     Document Type: Article

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