Successive merging of plasmoids and fragmentation in flare current sheet and their X-ray and radio signatures
M. Karlick\'y, M. B\'arta

TL;DR
This paper combines MHD and kinetic simulations to study plasmoid merging and fragmentation in solar flare current sheets, explaining observed X-ray emissions and radio spikes through energetic electron acceleration.
Contribution
It presents a novel kinetic-level simulation of plasmoid interactions and fragmentation, linking these processes to observable flare signatures.
Findings
Plasmoid merging efficiently accelerates electrons to hard X-ray energies.
Fragmentation during merging can produce narrowband radio spikes.
Simulated X-ray spectra match observed flare emissions.
Abstract
Based on our recent MHD simulations, first, a concept of the successive merging of plasmoids and fragmentation in the current sheet in the standard flare model is presented. Then, using a 2.5-D electromagnetic particle-in-cell model with free boundary conditions, these processes were modelled on the kinetic level of plasma description. We recognized the plasmoids which mutually interacted and finally merged into one large plasmoid. Between interacting plasmoids further plasmoids and current sheets on smaller and smaller spatial scales were formed in agreement with the fragmentation found in MHD simulations. During interactions (merging - coalescences) of the plasmoids the electrons were very efficiently accelerated and heated. We found that after a series of such merging processes the electrons in some regions reached the energies relevant for the emission in the hard X-ray range.…
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