Sunspot group tilt angles and the strength of the solar cycle

Astronomy and Astrophysics

Volumn 518, Issue 22, 2010, Pages

  Dasi Espuig, M ^a   Solanki, S K ^a,b   Krivova, N A ^a   Cameron, R ^a   Penuela T ^a,c,d  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b Kyung Hee University   (South Korea)

^c ST PETERSBURG STATE UNIVERSITY   (Russian Federation)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

Author keywords

Magnetic fields; Sun: activity; Sun: dynamo; Sunspots

Indexed keywords

ANGLE MEASUREMENT; DC GENERATORS; EXTRATERRESTRIAL ATMOSPHERES; INTERACTIVE DEVICES; MAGNETIC FIELDS; MAGNETIC FLUX; MOUNTINGS; SUN; TIME SERIES; UPPER ATMOSPHERE;

ACTIVE REGIONS; CONFIDENCE LEVELS; CORRELATION COEFFICIENT; FLUX TRANSPORT; IN-BUILDINGS; LATITUDINAL DISTRIBUTION; LINEAR RELATIONSHIPS; POLAR FIELDS; POLOIDAL FLUX; POSITIVE CORRELATIONS; SOLAR ACTIVITY; SOLAR CYCLE; SOLAR DYNAMO; SOURCE TERMS; SUN: ACTIVITY; SUN:DYNAMO; SUNSPOTS; TILT ANGLE; TILT ANGLE MEASUREMENT;

SOLAR ENERGY;

EID: 77957834836     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014301     Document Type: Article

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