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Quantifying the Influence of Key Physical Processes on the Formation of Emission Lines Observed by IRIS. I. Non-equilibrium Ionization and Density-dependent Rates
SI iv Resonance Line Emission during Solar Flares: Non-LTE, Nonequilibrium, Radiation Transfer Simulations
Graham S. Kerr, Mats Carlsson, Joel C. Allred, Peter R. Young and Adrian N. Daw The Astrophysical Journal 871(1) 23 (2019) https://doi.org/10.3847/1538-4357/aaf46e