Comparison of the sidereal angular velocity of subphotospheric layers and small bright coronal structures during the declining phase of solar cycle 23

Astronomy and Astrophysics

Volumn 504, Issue 2, 2009, Pages 589-594

  Zaatri, A ^a,b   Wohl H ^a   Roth, M ^a   Corbard, T ^b   Brajsa R ^c  

^a KIEPENHEUER INSTITUT FÜR SONNENPHYSIK   (Germany)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c UNIVERSITY OF ZAGREB   (Croatia)

Author keywords

Methods: data analysis; Sun: corona; Sun: helioseismology; Sun: rotation

Indexed keywords

AUTOMATIC METHOD; CORONAL ROTATION; CORONAL STRUCTURE; DIFFERENTIAL ROTATION; DISK IMAGES; DOPPLERGRAMS; LATITUDINAL GRADIENTS; LOCAL HELIOSEISMOLOGY; MAGNETIC FEATURES; METHODS: DATA ANALYSIS; NORTH-SOUTH ASYMMETRY; NORTHERN HEMISPHERES; RING DIAGRAM ANALYSIS; ROTATION RATE; ROTATION VELOCITY; SOLAR CYCLE; SOLAR PLASMA; SOUTHERN HEMISPHERE; SUBSURFACE LAYER; SUN: CORONA; SUN: HELIOSEISMOLOGY; SUN: ROTATION; TORSIONAL OSCILLATION;

ANGULAR VELOCITY; ATMOSPHERICS; DISKS (STRUCTURAL COMPONENTS); MAGNETOMETERS; ROTATION; SOLAR ENERGY; SOLAR WIND; UPPER ATMOSPHERE; VELOCITY MEASUREMENT;

SUN;

EID: 70349317176     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912130     Document Type: Article

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