Theoretical intensity ratios for some Fe XIII coronal lines
- 1 June 1973
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 30 (2) , 381-384
- https://doi.org/10.1007/bf00152669
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Proton collisional excitation in the ground configuration of Fe+12Solar Physics, 1973
- Collision Strengths for Electron Excitation of Coronal IonsPublished by Springer Nature ,1971
- Fine-Structure TransitionsThe Astrophysical Journal, 1968
- Classification and oscillator strengths of lines in the far vacuum ultra-violet spectrum of the iron period elementsJournal of Physics B: Atomic and Molecular Physics, 1968
- Some Intermediate Coupling Transition Probabilities in CA XV and fe XIIIThe Astrophysical Journal, 1967
- On the Theoretical Transition Probabilities of Certain Emission Lines of the Solar CoronaThe Astrophysical Journal, 1966
- A General Formula for the Estimation of Dielectronic Recombination Co-Efficients in Low-Density Plasmas.The Astrophysical Journal, 1965
- The spectrum of the solar coronaPlanetary and Space Science, 1964
- Rate of Collisional Excitation in Stellar Atmospheres.The Astrophysical Journal, 1962
- The calculation of the absolute strengths of spectral linesPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1949