RHESSI-20 Workshop: Preparing for the Next Decade in High-Energy Solar Physics Research

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

8 Jul 2021, 18:35

50m

Virtual

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.

Presentation materials

talk_kasparova.pdf