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Cited article:

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Plasma Diagnostics from Active Region and Quiet-Sun Spectra Observed by Hinode/EIS: Quantifying the Departures from a Maxwellian Distribution

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Predicting the Extreme Ultraviolet Radiation Environment of Exoplanets around Low-mass Stars: GJ 832, GJ 176, and GJ 436

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High-resolution Laboratory Measurements of Coronal Lines near the Fe ix Line at 171 Å

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

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Solar Physics 292 (8) (2017)
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KAPPA: A PACKAGE FOR SYNTHESIS OF OPTICALLY THIN SPECTRA FOR THE NON-MAXWELLIAN κ -DISTRIBUTIONS BASED ON THE CHIANTI DATABASE

Elena Dzifčáková, Jaroslav Dudík, Pavel Kotrč, František Fárník and Alena Zemanová
The Astrophysical Journal Supplement Series 217 (1) 14 (2015)
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DIVISION B COMMISSION 14 WORKING GROUP: ATOMIC DATA

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Proceedings of the International Astronomical Union 11 (T29A) 103 (2015)
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IMAGING AND SPECTROSCOPIC OBSERVATIONS OF A TRANSIENT CORONAL LOOP: EVIDENCE FOR THE NON-MAXWELLIANκ-DISTRIBUTIONS

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Signatures of the non-Maxwellianκ-distributions in optically thin line spectra

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Astronomy & Astrophysics 570 A124 (2014)
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