Observational evidence of the primary role played by photospheric motions in magnetic helicity transport before a filament eruption

Astronomy and Astrophysics

Volumn 433, Issue 2, 2005, Pages 683-690

  Romano, P ^a   Contarino, L ^b   Zuccarello, F ^a  

^a UNIVERSITY OF CATANIA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

Author keywords

Sun: activity; Sun: filaments; Sun: magnetic fields

Indexed keywords

ASTROPHYSICS; ATMOSPHERIC MOVEMENTS; IMAGE ANALYSIS; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; SOLAR RADIATION; SUN; ULTRAVIOLET RADIATION;

FILAMENT ERUPTIONS; KINK INSTABILITY; PHOTOSPHERIC MOTIONS; SOLAR CORONA;

ASTRONOMY;

EID: 16644393115     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041807     Document Type: Article

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