During solar flares a tremendous amount of magnetic energy is released and transported
through the Sun's atmosphere and out into the heliosphere. Despite over a century of study …

Solar flares are transient yet dramatic events in the atmosphere of the Sun, during which a
vast amount of magnetic energy is liberated. This energy is subsequently transported …

We present light curves and flares from a 7 day, multiwavelength observational campaign of
AU Mic, a young and active dM1e star with exoplanets and a debris disk. We report on 73 …

White-light stellar flares are now reported by the thousands in long-baseline, high-precision,
broad-band photometry from missions like Kepler, K2, and TESS. These observations are …

Coronal flare emission is commonly observed to decay on timescales longer than those
predicted by impulsively driven, one-dimensional flare loop models. This discrepancy is …

Here, we present the study of a compact emission source during an X1. 3 flare on 2022
March 30. Within a∼ 41 s period (17: 34: 48 UT to 17: 35: 29 UT), Interface Region Imaging …

Magnetic reconnection is believed to play an important role in the release and conversion of
energy among magnetized plasma systems. So far, we have been unable to understand …

We have systematically investigated ultraviolet (UV) emission from molecular hydrogen (H2)
using the Interface Region Imaging Spectrograph (IRIS), during three X-ray flares of C5. 1 …

Abstract Solar Dynamics Observatory (SDO)/Helioseismic and Magnetic Imager (HMI)
observations reveal a class of solar flares with substantial energy and momentum impacts in …

The bulk of solar flare energy is deposited in the chromosphere. Flare ribbons and footpoints
in the chromosphere therefore offer great diagnostic potential of flare energy release and …