Interpretation of multiwavelength observations of November 5, 1980 solar flares by the magnetic topology of AR 2766
We present a detailed analysis of the magnetic topology of AR 2776 together with H α UV, X-rays, and radio observations of the November 5, 1980 flares in order to understand the role of the active region large-scale topology on the flare process. As at present the coronal magnetic field is modeled b...
Publicado: |
1994
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Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v150_n1-2_p221_Demoulin http://hdl.handle.net/20.500.12110/paper_00380938_v150_n1-2_p221_Demoulin |
Aporte de: |
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