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...
Guardado en:
Autores principales: | Démoulin, P., Mandrini, C.H., Rovira, M.G., Hénoux, J.C., Machado, M.E. |
---|---|
Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v150_n1-2_p221_Demoulin |
Aporte de: |
Ejemplares similares
-
Interpretation of multiwavelength observations of November 5, 1980 solar flares by the magnetic topology of AR 2766
por: Démoulin, Pascal
Publicado: (1994) -
Interpretation of multiwavelength observations of November 5, 1980 solar flares by the magnetic topology of AR 2766
Publicado: (1994) -
Development of a topological model for solar flares
por: Démoulin, P., et al. -
Quasi-separatrix layers in solar flares: II. Observed magnetic configurations
por: Démoulin, P., et al. -
Observational support of reconnection in solar flares
por: Démoulin, P., et al.