Solar activity due to magnetic complexity of active regions
Active regions (ARs), involved in the Halloween events during October-November 2003, were the source of unusual activity during the following solar rotation. The flares on 18-20 November 2003 that occur in the AR NOAA10501 were accompanied by coronal mass ejections associated to some particularly ge...
Guardado en:
Autores principales: | Schmieder, B., Mandrini, C., Chandra, R., Démoulin, P., Török, T., Pariat, E., Uddin, W. |
---|---|
Formato: | Artículo publishedVersion |
Publicado: |
2010
|
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_17439213_v6_nS273_p164_Schmieder https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_17439213_v6_nS273_p164_Schmieder_oai |
Aporte de: |
Ejemplares similares
-
Solar activity due to magnetic complexity of active regions
por: Schmieder, B., et al.
Publicado: (2010) -
Solar activity due to magnetic complexity of active regions
por: Schmieder, B., et al. -
Solar activity due to magnetic complexity of active regions
por: Mandrini, Cristina Hemilse
Publicado: (2010) -
How can a negative magnetic helicity active region generate a positive helicity magnetic cloud?
por: Chandra, R., et al. -
Study of magnetic flux emergence and related activity in active region NOAA 10314
por: Poisson, M., et al.