Variability of EUV-spectra from the quiet upper solar atmosphere: Intensity and Doppler shift
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20030400/pdf
Reference33 articles.
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1. 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;The Astrophysical Journal;2015-03-13
2. Spectral analysis of 3D MHD models of coronal structures;Advances in Space Research;2009-05
3. 4.1.1.5 Solar transition region and quiet corona;Solar System;2009
4. Sizes of transition-region structures in coronal holes and in the quiet Sun;Astronomy & Astrophysics;2008-03-04
5. Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations;Space Science Reviews;2007-12
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