Description
We present indications of reconnection within the erupting flux rope which occurred during the impulsive phase of the Apr 2, 2022 flare. Combining data from ground-based radiospectrometers, EUV and X-ray data from different vantage points (STEREO, AIA/SDO, EUI/Solar Orbiter, STIX/Solar Orbiter, Fermi), we show that rare and unique radio bursts in the GHz frequency range are co-temporal with specific EUV structures. In addition, the X-ray sources are related to hot EUV loops and footpoints that are all located near or inside the magnetic rope and the erupting filament.
Primary authors
Jana Kasparova
Jaroslav Dudik
(Astronomical Institute of the Czech Academy of Sciences)
Marian Karlický
(Astronomical Institute ASCR)
Paolo Massa
(Dipartimento di Matematica, Università di Genova)
Sam Krucker
(FHNW School of Engineering)
Dr
Alena Zemanova
(Astronomical Institute, Czech Academy of Sciences)
