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Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI
M. E. Weller, P. Beiersdorfer, V. A. Soukhanovskii, F. Scotti and B. P. LeBlanc The Astrophysical Journal 854(2) 102 (2018) https://doi.org/10.3847/1538-4357/aaa5a1
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
S. V. Kuzin, S. A. Bogachev, A. M. Urnov, et al. Springer Series on Atomic, Optical, and Plasma Physics, Atomic Processes in Basic and Applied Physics 68 37 (2012) https://doi.org/10.1007/978-3-642-25569-4_3
INTENSITY RATIO OF DENSITY-SENSITIVE LINES IN Fe IONS OBSERVED WITH A WELL-DEFINED LABORATORY PLASMA
Emission lines of Na-like ions in spectra obtained with the Solar EUV Research Telescope and Spectrograph (SERTS)
F. P. Keenan, A. C. Katsiyannis, J. W. Brosius, J. M. Davila and R. J. Thomas Monthly Notices of the Royal Astronomical Society 342(2) 513 (2003) https://doi.org/10.1046/j.1365-8711.2003.06559.x
Astrophysics in 2002
Virginia Trimble and Markus J. Aschwanden Publications of the Astronomical Society of the Pacific 115(807) 514 (2003) https://doi.org/10.1086/374651