Speaker
Reetika Joshi
(NASA GSFC)
Description
Solar flares rapidly and energetically discharge magnetic energy in the solar atmosphere, accelerating charged particles to high velocities and generating intense bursts of radiation across the whole electromagnetic spectrum. Observing flares with high-resolution spectropolarimetric imaging from ground-based instruments remains challenging due to factors such as unpredictability of flares in small field of view, seeing conditions and weather limitations. We present observations of a solar flare from multi instruments and modelling using the state-of-the-art flare modeling, 1D radiation hydrodynamics (RADYN) code, to advance the comprehension of the dynamic solar atmosphere during flare eruption.
Primary author
Reetika Joshi
(NASA GSFC)
