The analysis of XUV emission lines
- 1 December 1975
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 45 (2) , 301-317
- https://doi.org/10.1007/bf00158452
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Relative coronal abundances derived from X-ray observations. III - The effect of cascades on the relative intensity of Fe XVII line fluxes, and a revised iron abundanceThe Astrophysical Journal, 1974
- Relative Coronal Abundances Derived from X-Ray Observations. IL Nitrogen, Oxygen, Neon, Magnesium, and IronThe Astrophysical Journal, 1974
- Relative Coronal Abundances Derived from X-Ray Observations. I. Sodium, Magnesium, Aluminum, Silicon, Sulfur, and ArgonThe Astrophysical Journal, 1974
- Models of the Chromospheric-Coronal Transition Layer and Lower Corona Derived from Extreme-Ultraviolet ObservationsThe Astrophysical Journal, 1973
- The Extreme-Ultraviolet Spectrum of a Solar Active RegionThe Astrophysical Journal, 1973
- Analysis of the Extreme-Ultraviolet Quiet Solar SpectrumThe Astrophysical Journal, 1972
- The Extreme-Ultraviolet Spectrum of the Quiet SunThe Astrophysical Journal, 1971
- Calculations of Ionization Equilibria for Oxygen, Neon, Silicon, and IronThe Astrophysical Journal, 1969
- Theoretical Line Intensities. V. Solar UV Emission Lines of Heavy ElementsThe Astrophysical Journal, 1966
- Excitation of lithium-like ions by electron impactsProceedings of the Physical Society, 1966