Theoretical intensities of Fexiv in the solar EUV spectrum
- 1 March 1971
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 17 (1) , 99-116
- https://doi.org/10.1007/bf00152865
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- Fine-Structure TransitionsThe Astrophysical Journal, 1968
- Highly ionized spectra of the transition elementsProceedings of the Physical Society, 1967
- New spectra of Fe XII to Fe XVIII and their isoelectronic sequencesProceedings of the Physical Society, 1967
- Coronal Emission-Line Intensities in the Extreme UltravioletThe Astrophysical Journal, 1966
- The Abundance of Iron in the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1966
- Delectronic Recombination and the Temperature of the Solar Corona.The Astrophysical Journal, 1964
- Excitation of Coronal Lines by Proton ImpactMonthly Notices of the Royal Astronomical Society, 1964
- L'excitation des atomes par chocs électroniquesAnnales de Physique, 1963
- The Self-Consistent Field with Exchange for the Ground State and First Excited State of Fe+13Monthly Notices of the Royal Astronomical Society, 1957
- Mg I- hnliche Spektren der Elemente Titan bis Cobalt, Ti XI, V XII, Cr XIII, Mn XIV, Fe XV und Co XVIThe European Physical Journal A, 1936