Study of the White-light Emission During the X9.3 Flare on September 06, 2017

Jul 8, 2021, 6:35 PM
50m
Virtual

Virtual

Connection details will be available soon
Working Group 1: Flare thermal response Working Group 1: Flare thermal response

Speaker

Jana Kasparova (Astronomical Institute of the CAS)

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.

Email jana.kasparova@asu.cas.cz

Primary authors

Jana Kasparova (Astronomical Institute of the CAS) Lucia Mravcova Michal Svanda Jan Jurcak Petr Heinzel

Presentation materials