Partially ionized plasma of the solar atmosphere: recent advances and future pathways
Author:
Affiliation:
1. Department of Mathematics and Statistics, University of Exeter, Exeter EX4 4QF, UK
2. Departament de Física and Institute of Applied Computing & Community Code (IAC3). Universitat de les Illes Balears, 07122 Palma de Mallorca (Spain)
Publisher
The Royal Society
Link
https://royalsocietypublishing.org/doi/pdf/10.1098/rsta.2023.0230
Reference12 articles.
1. Partial ionization of plasma in solar prominences;Heinzel P;Phil. Trans. R. Soc. A,2024
2. The influence of thermal pressure gradients and ionization (im)balance on the ambipolar diffusion and charge-neutral drifts;Gómez Míguez MM;Phil. Trans. R. Soc. A,2024
3. On the ambipolar diffusion formulation for ion-neutral drifts in the non-negligible drift velocity limit;Hillier AS;Phil. Trans. R. Soc. A,2024
4. Magnetohydrodynamic waves in the partially ionized solar plasma;Soler R;Phil. Trans. R. Soc. A,2024
5. Nonlinear coupling of Alfvén and magnetoacoustic waves in partially ionized plasmas: the effect of thermal misbalance on propagating waves;Ballester JL;Phil. Trans. R. Soc. A,2024
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