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Nonlinear coupling of Alfvén and magnetoacoustic waves in partially ionized plasmas: the effect of thermal misbalance on propagating waves
J. L. Ballester, R. Soler, J. Terradas and M. Carbonell Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 382(2272) (2024) https://doi.org/10.1098/rsta.2023.0222
Magnetohydrodynamic waves in the partially ionized solar plasma
Roberto Soler Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 382(2272) (2024) https://doi.org/10.1098/rsta.2023.0223
Viscous heating and instabilities in the partially ionized solar atmosphere
P. Hunana, T. Passot, E. Khomenko, D. Martínez-Gómez, M. Collados, A. Tenerani, G. P. Zank, Y. Maneva, M. L. Goldstein and G. M. Webb The Astrophysical Journal Supplement Series 260(2) 26 (2022) https://doi.org/10.3847/1538-4365/ac5044
Two-fluid Modeling of Acoustic Wave Propagation in Gravitationally Stratified Isothermal Media
Ion–neutral Interactions and Nonequilibrium Ionization in the Solar Chromosphere
Juan Martínez-Sykora, Jorrit Leenaarts, Bart De Pontieu, Daniel Nóbrega-Siverio, Viggo H. Hansteen, Mats Carlsson and Mikolaj Szydlarski The Astrophysical Journal 889(2) 95 (2020) https://doi.org/10.3847/1538-4357/ab643f
MHD waves in the collisional plasma of the solar corona and terrestrial ionosphere
Topics in Magnetohydrodynamic Topology, Reconnection and Stability Theory
Elena Khomenko CISM International Centre for Mechanical Sciences, Topics in Magnetohydrodynamic Topology, Reconnection and Stability Theory 591 69 (2020) https://doi.org/10.1007/978-3-030-16343-3_3
MHD WAVES IN THE COLLISIONAL PLASMA OF THE SOLAR CORONA AND TERRESTRIAL IONOSPHERE
The role of partial ionization effects in the chromosphere
Juan Martínez-Sykora, Bart De Pontieu, Viggo Hansteen and Mats Carlsson Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 373(2042) 20140268 (2015) https://doi.org/10.1098/rsta.2014.0268
Overdamped Alfvén waves due to ion-neutral collisions in the solar chromosphere