Speaker
Jana Kasparova
Description
Using data from SDO/HMI, Hinode/SOT, and LYRA instruments, we study the white-light continuum emission during the X9.3 solar flare (SOL2017-09-06T11:53). Assuming that the emission is due to hydrogen Balmer and Paschen continua, we estimate the temperature evolution during that solar flare.
Primary author
Jana Kasparova
Co-authors
Lucia Mravcova
Dr
Michal Svanda
Dr
Jan Jurcak
Dr
Petr Heinzel
(Observatoire De Ondrejov)
