Pregled bibliografske jedinice broj: 863652
Estimation of the back-illumination of the chromosphere for the 2011-02-15 flare
Estimation of the back-illumination of the chromosphere for the 2011-02-15 flare // Coronal Loop Workshop VII - Heating of the Magnetically Closed Corona / Helen Mason (ur.).
Cambridge, 2015. str. 34-35 (poster, nije recenziran, sažetak, znanstveni)
CROSBI ID: 863652 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Estimation of the back-illumination of the chromosphere for the 2011-02-15 flare
Autori
Skender, Marina ; Andretta, Vincenzo ; Varady, Michal, Heinzl, Petr
Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni
Izvornik
Coronal Loop Workshop VII - Heating of the Magnetically Closed Corona
/ Helen Mason - Cambridge, 2015, 34-35
Skup
Coronal Loop Workshop VII - Heating of the Magnetically Closed Corona
Mjesto i datum
Cambridge, Ujedinjeno Kraljevstvo, 21.07.2015. - 23.07.2015
Vrsta sudjelovanja
Poster
Vrsta recenzije
Nije recenziran
Ključne riječi
coronal loops, chromosphere, solar flares
(koronine petlje, kromosfera, Sunčevi bljeskovi)
Sažetak
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.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
