Particle Acceleration In Plasmoid Ejections Derived From Radio Drifting Pulsating Structures
N. Nishizuka, M. Karlicky, M. Janvier, M. Barta

TL;DR
This study analyzes radio spectrograph data to classify drifting pulsating structures (DPS) in solar flares, linking them to plasmoid ejections, particle acceleration, and magnetic reconnection processes.
Contribution
It provides a detailed classification of DPS events and correlates their spectral features with physical parameters of plasmoid ejections and reconnection rates.
Findings
DPS events are often associated with X-ray bursts.
Constant frequency drift indicates constant plasmoid velocity.
Reconnection rate correlates positively with plasmoid velocity.
Abstract
We report observations of slowly drifting pulsating structures (DPS) in the 0.8-4.5 GHz frequency range of the RT4 and RT5 radio spectrographs at Ondrejov observatory, between 2002 and 2012. We found 106 events of drifting pulsating structures, which we classified into 4 cases: (I) single events with a constant frequency drift [12 events], (II) multiple events occurring in the same flare with constant frequency drifts [11 events], (III) single or multiple events with increasing or decreasing frequency drift rates [52 events], and (IV) complex events containing multiple events occurring at the same time in the different frequency range [31 events]. Many DPSs are associated with hard X-ray bursts (15-25 keV) and soft X-ray gradient peaks, as they typically occurred at the beginning of the hard X-ray peaks. This indicates that DPS events are related to the processes of fast energy release…
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