Origin of the 30 THz Emission Detected During the Solar Flare on 2012 March 13 at 17:20 UT
Solar observations in the infrared domain can bring important clues on the response of the low solar atmosphere to primary energy released during flares. At present, the infrared continuum has been detected at 30 THz (10 μm) in only a few flares. SOL2012-03-13, which is one of these flares, has been...
Guardado en:
Autores principales: | Trottet, G., Raulin, J.-P., Mackinnon, A., Giménez de Castro, G., Simões, P.J.A., Cabezas, D., de La Luz, V., Luoni, M., Kaufmann, P. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00380938_v290_n10_p2809_Trottet |
Aporte de: |
Ejemplares similares
-
Origin of the 30 THz Emission Detected During the Solar Flare on 2012 March 13 at 17:20 UT
Publicado: (2015) -
Origin of the submillimeter radio emission during the time-extended phase of a solar flare
por: Trottet, G., et al. -
Origin of the submillimeter radio emission during the time-extended phase of a solar flare
por: Luoni, Maria Luisa
Publicado: (2012) -
Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare
por: Trottet, G., et al. -
Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare
por: Giménez de Castro, Carlos Guillermo, et al.
Publicado: (2011)