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Cited article:

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ELECTRON ENERGY PARTITION IN THE ABOVE-THE-LOOPTOP SOLAR HARD X-RAY SOURCES

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IMAGING AND SPECTROSCOPIC OBSERVATIONS OF A TRANSIENT CORONAL LOOP: EVIDENCE FOR THE NON-MAXWELLIANκ-DISTRIBUTIONS

Jaroslav Dudík, Šimon Mackovjak, Elena Dzifčáková, et al.
The Astrophysical Journal 807 (2) 123 (2015)
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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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THEORY OF GYRORESONANCE AND FREE-FREE EMISSIONS FROM NON-MAXWELLIAN QUASI-STEADY-STATE ELECTRON DISTRIBUTIONS

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The Astrophysical Journal 781 (2) 77 (2014)
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On the Possibility to Diagnose the Non-Maxwellian κ-Distributions from the Hinode/EIS EUV Spectra

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H TO Zn IONIZATION EQUILIBRIUM FOR THE NON-MAXWELLIAN ELECTRON κ-DISTRIBUTIONS: UPDATED CALCULATIONS

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The non-Maxwellian continuum in the X-ray, UV, and radio range

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Astronomy & Astrophysics 539 A107 (2012)
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Is it possible to model observed active region coronal emission simultaneously in EUV and X-ray filters?

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The bound-bound and free-free radiative losses for the nonthermal distributions in solar and stellar coronae

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Energy Storage and Release through the Solar Activity Cycle

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Multi-scale Physics in Coronal Heating and Solar Wind Acceleration

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Space Sciences Series of ISSI, Multi-scale Physics in Coronal Heating and Solar Wind Acceleration 38 315 (2011)
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