Excitation and evolution of coronal oscillations in self-consistent 3D radiative MHD simulations of the solar atmosphere - Kohutova, P.; Popovas, A. (Astronomy and astrophysics (Berlin), 2021)
Keywords: Atmospheric models; Computational fluid dynamics; Coronal loops; Damping; Emission analysis; Evolution; Excitation; Fluid flow; Harmonics; Helioseismology; Magnetic fields; Magnetic flux; Magnetohydrodynamics; Oscillations; Physical properties; Power spectra; Simulation; Solar atmosphere; Solar corona; Topology; Tubes; Ultraviolet emission