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.
A neural network detector applied to 2011 solar radio spectra identified 50 QFP wave train candidates, with 13 associated with global coronal EUV waves.
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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Detector for fast wave trains in the solar radio emission
A neural network detector applied to 2011 solar radio spectra identified 50 QFP wave train candidates, with 13 associated with global coronal EUV waves.