Recurrent coronal jets show QPPs of 6-13 min periods driven by periodic reconnection, with flux periodicities and sub-cooling timescales implying persistent localized heating in fan-spine structures.
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This review summarizes particle acceleration models in solar flares and how SKAO observations will enable better characterization of nonthermal particle populations and coronal properties.
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Recurrent Coronal Jets and QPPs: Periodic Reconnection and Localized Heating Across Quiet-Sun to Active Regions
Recurrent coronal jets show QPPs of 6-13 min periods driven by periodic reconnection, with flux periodicities and sub-cooling timescales implying persistent localized heating in fan-spine structures.
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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.