Observational evidence of the primary role played by photospheric motions in magnetic helicity transport before a filament eruption
- Author
- ROMANO, P1 ; CONTARINO, L2 ; ZUCCARELLO, F1
[1] Dipartimento di Fisica e Astronomia - Sezione Astrofisica, Università di Catania, via S. Sofia 78, 95125 Catania, Italy
[2] INAF - Osservatorio Astrofisico di Catania, via S. Sofia 78, 95125 Catania, Italy - Source
Astronomy and astrophysics (Berlin. Print). 2005, Vol 433, Num 2, pp 683-690, 8 p ; ref : 23 ref
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- Sun: activity Sun: filaments Sun: magnetic fields
- Keyword (fr)
- Champ magnétique Corde flux Filament Flux magnétique Hélicité Instabilité coque Magnétogramme Modèle Paramètre géométrique Soleil
- Keyword (en)
- Magnetic fields Flux rope Filaments Magnetic flux Helicity Kink instability Magnetogram Models Geometrical parameter Sun
- Keyword (es)
- Cuerda flujo Magnetograma Modelo Parámetro geométrico
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16645972
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1051/0004-6361:20041807 
https://dx.doi.org/10.1051/0004-6361:20041807
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