Density dependence of solar emission lines of oxygen-like ions
- 1 December 1978
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 60 (2) , 269-277
- https://doi.org/10.1007/bf00156527
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Prediction and Identification of Some Transitions Associated with 2pkand 2pk-13l Configurations in Six-, Seven- and Eight-electron IonsPhysica Scripta, 1977
- Radiation from a hot, thin plasma from 1 to 250 AThe Astrophysical Journal Supplement Series, 1976
- Density dependence of the line emission of boron-like coronal ionsAstrophysics and Space Science, 1975
- The Excitation of Several Iron and Calcium Lines in the Visible Spectrum of the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1975
- Forbidden-line excitation data for certain coronal linesThe Astrophysical Journal Supplement Series, 1974
- Z-dependence of the level intervals in 2s 2 2p 2, 2s 2 2p 3 and 2s 2 2p 4Solar Physics, 1972
- Theoretical intensities of Fexiv in the solar EUV spectrumSolar Physics, 1971
- The Relative Intensities of Lines from Bei-Like Ions in the Solar SpectrumPublished by Springer Nature ,1971
- The Ionization Equilibrium of Elements Between Carbon and NickelMonthly Notices of the Royal Astronomical Society, 1969
- Resonance lines of argon XI and XII and krypton IX and XProceedings of the Physical Society, 1964