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Cited article:

Extreme Red-wing Enhancements of UV Lines during the 2022 March 30 X1.3 Solar Flare

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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

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A Si iv/O iv Electron Density Diagnostic for the Analysis of IRIS Solar Spectra

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The Astrophysical Journal 857 (1) 5 (2018)
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Non-Maxwellian Analysis of the Transition-region Line Profiles Observed by the Interface Region Imaging Spectrograph

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Nonequilibrium Processes in the Solar Corona, Transition Region, Flares, and Solar Wind (Invited Review)

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Density diagnostics derived from the O iv and S iv intercombination lines observed by IRIS

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SLIPPING MAGNETIC RECONNECTION, CHROMOSPHERIC EVAPORATION, IMPLOSION, AND PRECURSORS IN THE 2014 SEPTEMBER 10 X1.6-CLASS SOLAR FLARE

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EXPLOSIVE EVENTS ON A SUBARCSECOND SCALE INIRISOBSERVATIONS: A CASE STUDY

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The Astrophysical Journal 797 (2) 88 (2014)
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Signatures of the non-Maxwellianκ-distributions in optically thin line spectra

J. Dudík, G. Del Zanna, H. E. Mason and E. Dzifčáková
Astronomy & Astrophysics 570 A124 (2014)
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Differential emission measure analysis of active region cores and quiet Sun for the non-Maxwellianκ-distributions

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Astronomy & Astrophysics 564 A130 (2014)
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SOLAR TRANSITION REGION LINES OBSERVED BY THE INTERFACE REGION IMAGING SPECTROGRAPH : DIAGNOSTICS FOR THE O IV AND Si IV LINES

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The Astrophysical Journal 780 (1) L12 (2013)
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