Realistic 3D MHD modeling of observed active region AR 11166 reproduces key observed properties of quasi-periodic fast propagating magnetosonic waves with improved qualitative agreement over idealized setups.
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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.
New observations of ~160 s VLPs in metric type-I bursts show spatiotemporal correlation with ~170 s oscillations in sunspot umbrae, supporting modulation by slow magnetoacoustic waves via plasma emission.
citing papers explorer
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Modeling the Excitation, Propagation and Damping of Quasi-Periodic Fast Magnetosonic Waves in Realistic Coronal Active Region Magnetic Field Structures
Realistic 3D MHD modeling of observed active region AR 11166 reproduces key observed properties of quasi-periodic fast propagating magnetosonic waves with improved qualitative agreement over idealized setups.
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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.
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Spatio-temporal Characteristics of Very Long-periodic Pulsations in Solar Metrewave Bursts: Implications for their Origins
New observations of ~160 s VLPs in metric type-I bursts show spatiotemporal correlation with ~170 s oscillations in sunspot umbrae, supporting modulation by slow magnetoacoustic waves via plasma emission.