The 8.2 μm mid-IR channel in solar flare footpoints peaks 0.3-0.45 s before the 5.2 μm channel due to wavelength-dependent opacity changes from flare-induced ionization.
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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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First time delay observation between two mid-infrared channels in solar flare footpoints
The 8.2 μm mid-IR channel in solar flare footpoints peaks 0.3-0.45 s before the 5.2 μm channel due to wavelength-dependent opacity changes from flare-induced ionization.
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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.