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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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.