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Effects of different coronal hole geometries on simulations of the interaction between coronal waves and coronal holes
I. Piantschitsch, J. Terradas, E. Soubrie, S. G. Heinemann, S. J. Hofmeister, R. Soler and M. Temmer Astronomy & Astrophysics 687 A200 (2024) https://doi.org/10.1051/0004-6361/202348003
Three-dimensional solar active region magnetohydrostatic models and their stability using Euler potentials
Standing Sausage Perturbations in Solar Coronal Slabs with Continuous Transverse Density Profiles: Cutoff Wavenumbers, Evanescent Eigenmodes, and Oscillatory Continuum