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Non-local thermodynamic equilibrium inversions of the Si I 10827 Å spectral line
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Damping of coronal oscillations in self-consistent 3D radiative magnetohydrodynamics simulations of the solar atmosphere
Scalable matrix-free solver for 3D transfer of polarized radiation in stellar atmospheres
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C. Quintero Noda, R. Schlichenmaier, L. R. Bellot Rubio, et al. Astronomy & Astrophysics 666 A21 (2022) https://doi.org/10.1051/0004-6361/202243867
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The First 3D Coronal Loop Model Heated by MHD Waves against Radiative Losses
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A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)
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The Effects of Three-dimensional Radiative Transfer on the Resonance Polarization of the Ca i 4227 Å Line
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New Light on an Old Problem of the Cores of Solar Resonance Lines
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Physical properties of bright Ca II K fibrils in the solar chromosphere
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Cosmic-ray interactions with the Sun using the fluka code