Simulations demonstrate that fast magnetoacoustic waves incident on a localized coronal null undergo mode conversion to produce incompressible energetic Alfvén wave packets along separatrices.
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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.
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Interaction of Fast Magnetoacoustic Wave with the Localized Coronal Null and Generation of the Energetic Alfv\'en Wave Packet
Simulations demonstrate that fast magnetoacoustic waves incident on a localized coronal null undergo mode conversion to produce incompressible energetic Alfvén wave packets along separatrices.
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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.