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.
Title resolution pending
2 Pith papers cite this work, alongside 15 external citations. Polarity classification is still indexing.
2
Pith papers citing it
15
external citations · OpenAlex
fields
astro-ph.SR 2representative citing papers
Two oppositely directed fast-mode wave trains from an M6.0 flare show matching ~66–75 s periods, and their speeds yield magnetic-field estimates that only partially overlap with magnetic extrapolation values.
citing papers explorer
-
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.
-
Multi-Path Quasi-Periodic Fast-mode Propagating Magnetoacoustic Waves to Diagnose Coronal Magnetic Field and Flaring Core
Two oppositely directed fast-mode wave trains from an M6.0 flare show matching ~66–75 s periods, and their speeds yield magnetic-field estimates that only partially overlap with magnetic extrapolation values.