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Cited article:

Diagnostics of Non-Maxwellian Electron Distributions in Solar Active Regions from Fe xii Lines Observed by the Hinode Extreme Ultraviolet Imaging Spectrometer and Interface Region Imaging Spectrograph

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Electron Densities in the Solar Corona Measured Simultaneously in the Extreme Ultraviolet and Infrared

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KAPPA: A Package for the Synthesis of Optically Thin Spectra for the Non-Maxwellian κ-distributions. II. Major Update to Compatibility with CHIANTI Version 10

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CHIANTI—An Atomic Database for Emission Lines. XVI. Version 10, Further Extensions

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Large-scale Multiconfiguration Dirac–Hartree–Fock Calculations for Astrophysics: n = 4 Levels in P-like Ions from Mn xi to Ni xiv

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Laboratory Calibrations of Fe xii–xiv Line-intensity Ratios for Electron Density Diagnostics

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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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Energy Levels, Lifetimes, and Transition Rates for P-like Ions from Cr x to Zn xvi from Large-scale Relativistic Multiconfiguration Calculations

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G Y Liang, H G Wei, G Zhao and J Y Zhong
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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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CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XIII. SOFT X-RAY IMPROVEMENTS AND OTHER CHANGES

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Doppler shift of hot coronal lines in a moss area of an active region

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