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astro-ph.SR2024
Fe I 6173 Å Emission During White-Light Solar Flares
Samuel Granovsky, Alexander G. Kosovichev, Viacheslav M. Sadykov +2
Between 2017 and 2024, the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory has observed numerous white-light solar flares (WLFs). HMI spectro-polarime…
astro-ph.SR2024
Solar Flare Ribbon Fronts. II. Evolution of heating rates in individual flare footpoints
Graham S. Kerr, Vanessa Polito, Yan Xu +1
Solar flare ribbon fronts appear ahead of the bright structures that normally characterise solar flares, and can persist for an extended period of time in spatially localised patch…