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Cited article:

Synthetic Spectra of the Fe VIII  – Fe XVI Emission Lines for Electron Non-Thermal Distributions

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CHIANTI—An Atomic Database for Emission Lines. VI. Proton Rates and Other Improvements

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The Astrophysical Journal Supplement Series 144 (1) 135 (2003)
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A Comparison between Coronal Emission Lines from an Isothermal Spectrum Observed with the Coronal Diagnostic Spectrometer and CHIANTI Emissivities

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Collisions of Electrons with Atomic Ions

A. K. Pradhan and H. L. Zhang
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CHIANTI—An Atomic Database for Emission Lines. V. Comparison with an Isothermal Spectrum Observed with SUMER

E. Landi, U. Feldman and K. P. Dere
The Astrophysical Journal Supplement Series 139 (1) 281 (2002)
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Collisions of Electrons with Atomic Ions

A. K. Pradhan and H. L. Zhang
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Collisions of Electrons with Atomic Ions

A. K. Pradhan and H. L. Zhang
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A comparison between theoretical and solar FeXII UV line intensity ratios

A. M. Binello, E. Landi, H. E. Mason, P. J. Storey and J. W. Brosius
Astronomy & Astrophysics 370 (3) 1071 (2001)
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Fe xii emission lines in solar active regions observed by the RES-C spectroheliograph on the CORONAS-I mission

I. A. Zhitnik, S. V. Kuzin, A. M. Urnov, F. P. Keenan and D. J. Pinfield
Monthly Notices of the Royal Astronomical Society 308 (1) 228 (1999)
https://doi.org/10.1046/j.1365-8711.1999.02756.x