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Published in 2024 at "Research in Astronomy and Astrophysics"
DOI: 10.1088/1674-4527/ad9255
Abstract: The propagation of disturbances in the solar atmosphere is inherently three-dimensional (3D), yet comprehensive studies on the spatial structure and dynamics of 3D wave fronts are scarce. Here we conduct high-resolution 3D numerical simulations to…
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Keywords:
fast mode;
anisotropy qfp;
flux rope;
components anisotropy ... See more keywords