Estimation of the back-illumination of the chromosphere for the 2011-02-15 flare (CROSBI ID 645510)
Prilog sa skupa u zborniku | sažetak izlaganja sa skupa
Podaci o odgovornosti
Skender, Marina ; Andretta, Vincenzo ; Varady, Michal, Heinzl, Petr
engleski
Estimation of the back-illumination of the chromosphere for the 2011-02-15 flare
One of the main ingredients of the energetics of the flaring chromosphere is back-illumination from the flaring corona. In the recent time observational data became available, which can be used as empirical constrain for the back-illumination. In this study the EUV heating of the solar chromosphere is inferred in gradual phase of the flare 2011-02-15. Overlying EUV loops are assumed to have a semi-circular static symmetric configuration. SDO AIA and EVE data are utilised for estimating the spatial and spectral distribution of the EUV emitter sources. Further modelling is performed by the FLARIX code. Preliminary inferring of the energetics of the EUV coronal back-illumination is presented.
koronine petlje, kromosfera, Sunčevi bljeskovi
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Podaci o prilogu
34-35.
2015.
objavljeno
Podaci o matičnoj publikaciji
Coronal Loop Workshop VII - Heating of the Magnetically Closed Corona
Helen Mason
Cambridge:
Podaci o skupu
Coronal Loop Workshop VII - Heating of the Magnetically Closed Corona
poster
21.07.2015-23.07.2015
Cambridge, Ujedinjeno Kraljevstvo