Two-fluid implementation in MPI-AMRVAC with applications to the solar chromosphere
Context. The chromosphere is a partially ionized layer of the solar atmosphere, which acts as the transition between the photosphere where the gas is almost neutral and the fully ionized corona. As the collisional coupling between neutral and charged particles decreases in the upper part of the chro...
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| Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2022-08, Vol.664, p.A55 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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