Investigating the variation of latitudinal stellar spot rotation and its relation to the real stellar surface rotation

Astronomy and Astrophysics

Volumn 532, Issue , 2011, Pages

  Korhonen, H ^a,b   Elstner, D ^c  

^a UNIVERSITY OF TURKU   (Finland)

^b KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^c ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

Author keywords

Magnetic fields; Magnetohydrodynamics (MHD); Stars: activity; Stars: rotation; Starspots

Indexed keywords

ACTIVITY CYCLES; DIFFERENTIAL ROTATION; DOPPLER IMAGING TECHNIQUES; DYNAMO CALCULATIONS; DYNAMO MODELS; DYNAMO SIMULATION; GEOMETRIC PROPERTIES; MAGNETIC PATTERNS; MAGNETIC PRESSURE; MAGNETOHYDRODYNAMICS (MHD); ROTATION PATTERN; SIMILAR ANALYSIS; STARS: ACTIVITY; STARS: ROTATION; STARSPOTS; STELLAR SURFACES; SURFACE DIFFERENTIALS; SURFACE FLOW PATTERNS; SURFACE ROTATION; TEMPERATURE MAPS; TIME POINTS;

ELECTRIC GENERATORS; IMAGING TECHNIQUES; INTERACTIVE DEVICES; INVESTMENTS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; SOLAR SYSTEM; STARS;

ROTATION;

EID: 79961119022     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117016     Document Type: Article

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