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Cited article:

SYNTHESIZED SPECTRA OF OPTICALLY THIN EMISSION LINES PRODUCED BY THE BIFROST STELLAR ATMOSPHERE CODE, INCLUDING NONEQUILIBRIUM IONIZATION EFFECTS: A STUDY OF THE INTENSITY, NONTHERMAL LINE WIDTHS, AND DOPPLER SHIFTS

K. Olluri, B. V. Gudiksen, V. H. Hansteen and B. De Pontieu
The Astrophysical Journal 802 (1) 5 (2015)
https://doi.org/10.1088/0004-637X/802/1/5

Sizes of transition-region structures in coronal holes and in the quiet Sun

H. Tian, E. Marsch, C.-Y. Tu, L.-D. Xia and J.-S. He
Astronomy & Astrophysics 482 (1) 267 (2008)
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Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations

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Space Science Reviews 133 (1-4) 103 (2007)
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Forward Modeling of the Corona of the Sun and Solar‐like Stars: From a Three‐dimensional Magnetohydrodynamic Model to Synthetic Extreme‐Ultraviolet Spectra

Hardi Peter, Boris V. Gudiksen and Ake Nordlund
The Astrophysical Journal 638 (2) 1086 (2006)
https://doi.org/10.1086/499117

Astrophysics in 2003

Virginia Trimble and Markus J. Aschwanden
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Hida Domeless Solar Telescope andSOHOCoronal Diagnostic Spectrometer Observations of Short‐Duration Active Region Blinkers. II. Extreme‐Ultraviolet Properties

D. H. Brooks and H. Kurokawa
The Astrophysical Journal 611 (2) 1125 (2004)
https://doi.org/10.1086/422189