How numerical treatments of the transition region modify energy flux into the solar corona

The large temperature gradients in the solar transition region present a significant challenge to large scale numerical modelling of the Sun's atmosphere. In response, a variety of techniques have been developed which modify the thermodynamics of the system. This sacrifices accuracy in the tran...

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Veröffentlicht in:	arXiv.org 2023-09
Hauptverfasser:	Howson, Thomas, Breu, Cosima
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheric models Energy Heating Lower atmosphere Magnetohydrodynamic waves Numerical models One dimensional models Resonant frequencies Solar atmosphere Solar corona Solar transition region Thermodynamics Tracking Travel time
Online-Zugang:	Volltext
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