Decayless kink oscillations in coronal loops maintain stable amplitudes despite nearby solar flares of various classes.
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Superposition of standing slow and entropy modes in a 1D coronal loop with thermal conduction produces non-exponential damping and phase shifts in compressive oscillations.
citing papers explorer
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Effect of Solar Flares on Decayless Kink Oscillations in Nearby Coronal Loops
Decayless kink oscillations in coronal loops maintain stable amplitudes despite nearby solar flares of various classes.
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Entropy-mode imprints in the solar corona: non-exponential damping and phase shifts of compressive oscillations
Superposition of standing slow and entropy modes in a 1D coronal loop with thermal conduction produces non-exponential damping and phase shifts in compressive oscillations.