Fast magneto-acoustic waves in the solar chromosphere: Comparison of single-fluid and two-fluid approximations
Context. The mechanism behind the heating of the solar chromosphere remains unclear. Friction between neutrals and charges is expected to contribute to plasma heating in a partially ionised plasma (PIP). Aims. We aim to study the efficiency of the frictional heating mechanism in partially ionised plasmas by comparing a single-fluid model (1F) using
Gómez-Míguez, M. M. et al.
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9
2025