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Cited article:

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RAPID EVOLUTION OF THE SOLAR ATMOSPHERE DURING THE IMPULSIVE PHASE OF A MICROFLARE OBSERVED WITH THE EXTREME-ULTRAVIOLET IMAGING SPECTROMETER ABOARDHINODE: HINTS OF CHROMOSPHERIC MAGNETIC RECONNECTION

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INTENSITY RATIO OF DENSITY-SENSITIVE LINES IN Fe IONS OBSERVED WITH A WELL-DEFINED LABORATORY PLASMA

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The Astrophysical Journal 739 (1) 17 (2011)
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Measurement and Modeling of Density‐Sensitive Lines of Fexiiiin the Extreme Ultraviolet

N. Yamamoto, T. Kato, H. Funaba, et al.
The Astrophysical Journal 689 (1) 646 (2008)
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Solar EUV spectra obtained during the SPIRIT experiment onboard the CORONAS-F satellite: A catalog of lines in the range 176–207 Å

S. V. Shestov, S. A. Bozhenkov, I. A. Zhitnik, et al.
Astronomy Letters 34 (1) 33 (2008)
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Fe xiii emission lines in active region spectra obtained with the Solar Extreme-Ultraviolet Research Telescope and Spectrograph

F. P. Keenan, D. B. Jess, K. M. Aggarwal, et al.
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Emission lines of Na-like ions in spectra obtained with the Solar EUV Research Telescope and Spectrograph (SERTS)

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https://doi.org/10.1046/j.1365-8711.2003.06559.x

Astrophysics in 2002

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