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.
Non-relativistic Gaunt factors
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MUSE observations of Tc 1 map structured extinction, Te, and Ne, revealing a low-extinction annulus outside the main fullerene zone that is interpreted as evidence for locally altered dust properties in the core-halo transition.
citing papers explorer
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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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MUSE Imaging Spectroscopy of the Fullerene Planetary Nebula Tc 1
MUSE observations of Tc 1 map structured extinction, Te, and Ne, revealing a low-extinction annulus outside the main fullerene zone that is interpreted as evidence for locally altered dust properties in the core-halo transition.