This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.
Electron acceleration in three-dimensional magnetic reconnection with a guide field
1 Pith paper cite this work, alongside 119 external citations. Polarity classification is still indexing.
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Pith paper citing it
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abstract
Kinetic simulations of 3D collisionless magnetic reconnection with a guide field show a dramatic enhancement of energetic electron production when compared with 2D systems. In the 2D systems, electrons are trapped in magnetic islands that limit their energy gain, whereas in the 3D systems the filamentation of the current layer leads to a stochastic magnetic field that enables the electrons to access volume-filling acceleration regions. The dominant accelerator of the most energetic electrons is a Fermi-like mechanism associated with reflection of charged particles from contracting field lines.
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Radio Diagnostics of Particle Acceleration in Solar Flares with SKAO Observations
This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.