Spatial characterization of a flare using radio observations and magnetic field topology
Using magnetograms, EUV and Hα images, Owens Valley Solar Array microwave observations, and 212-GHz flux density derived from the Solar Submillimeter Telescope data, we determine the spatial characteristics of the 1B/M6.9 flare that occurred on November 28, 2001, starting at 16:26 UT in active regio...
Guardado en:
Autores principales: | Cristiani, G., Martinez, G., Mandrini, C.H., Giménez De Castro, C.G., Da Silva, C.W., Rovira, M.G., Kaufmann, P. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v240_n2_p271_Cristiani |
Aporte de: |
Ejemplares similares
-
Spatial characterization of a flare using radio observations and magnetic field topology
Publicado: (2007) -
Physical Processes Involved in the EUV “Surge” Event of 9 May 2012
por: López Fuentes, M., et al. -
Physical Processes Involved in the EUV “Surge” Event of 9 May 2012
Publicado: (2018) -
Observational support of reconnection in solar flares
por: Démoulin, P., et al. -
Observational support of reconnection in solar flares
Publicado: (1994)