Fe XIII line intensities in solar plasmas observed by SERTS
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20011705/pdf
Reference32 articles.
1. A comparison between theoretical and solar FeXII UV line intensity ratios
2. New model of iron spectra in the extreme ultraviolet and application to SERTS and EUV observations: A solar active region and capella
3. Measuring Active and Quiet-Sun Coronal Plasma Properties with Extreme-Ultraviolet Spectra from SERTS
4. Solar Active Region and Quiet‐Sun Extreme‐Ultraviolet Spectra from SERTS‐95
5. Analysis of a Solar Active Region Extreme‐Ultraviolet Spectrum from SERTS‐97
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1. Solar UV and X-ray spectral diagnostics;Living Reviews in Solar Physics;2018-08-31
2. Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI;The Astrophysical Journal;2018-02-15
3. 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;The Astrophysical Journal;2013-10-22
4. Large Hot X-Ray Sources in the Solar Corona;Atomic Processes in Basic and Applied Physics;2012
5. INTENSITY RATIO OF DENSITY-SENSITIVE LINES IN Fe IONS OBSERVED WITH A WELL-DEFINED LABORATORY PLASMA;The Astrophysical Journal;2011-08-30
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