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Simulation of emission of the flare 27.04.2012 in spectral lines of Hydrogen, Helium and Calcium
Yu.A. Kupryakov, K.V. Bychkov, O.M. Belova, V. A. Maliutin and A.B. Gorshkov Vestnik Moskovskogo Universiteta, Seriya 3: Fizika, Astronomiya (№2_2024) 2420801–1 (2024) https://doi.org/10.55959/MSU0579-9392.79.2420801
Simulation of the April 27, 2012 Flare Emission in the Spectral Lines of Hydrogen, Helium, and Calcium
Yu. A. Kupryakov, K. V. Bychkov, O. M. Belova, V. A. Maliutin and A. B. Gorshkov Moscow University Physics Bulletin 79(2) 275 (2024) https://doi.org/10.3103/S0027134924700334
1.5D non-LTE spectral synthesis of a 3D filament and prominence simulation
On the importance of Ca ii photoionization by the hydrogen lyman transitions in solar flare models
C M J Osborne, P Heinzel, J Kašparová and L Fletcher Monthly Notices of the Royal Astronomical Society 507(2) 1972 (2021) https://doi.org/10.1093/mnras/stab2156
Spectral Diagnostics of Cool Flare Loops Observed by the SST. I. Inversion of the Ca ii 8542 Å and Hβ Lines
Thomas Rimmele, Thomas Berger, Roberto Casini, et al. Proceedings of the International Astronomical Union 8(S300) 362 (2013) https://doi.org/10.1017/S1743921313011204
Radiative equilibrium in solar prominences reconsidered