A Critical Survey of the Low Configurations in Be I-like Spectra
- 1 August 1979
- journal article
- Published by IOP Publishing in Physica Scripta
- Vol. 20 (2) , 129-137
- https://doi.org/10.1088/0031-8949/20/2/001
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Accurate Semi-Empirical Formulae for the Energy Structure of Li I-like SpectraPhysica Scripta, 1979
- Spectral lines observed in solar flares between 171 and 630 angstromsThe Astrophysical Journal, 1978
- The solar spectrum - Wavelengths and identifications from 160 to 770 angstromsThe Astrophysical Journal, 1976
- Wavelengths and classifications of emission lines due to 2s22pn−2s2pn + 1 and 2s2pn−2pn + 1 transitions, Z ≤ 28Atomic Data and Nuclear Data Tables, 1975
- Classification of Spectra of K, Ca, Sc, Ti, V and Cr and Extrapolation to Fe Solar Flare LinesMonthly Notices of the Royal Astronomical Society, 1975
- Solar-flare emission lines in the range from 66 to 171 A; transitions in highly ionized iron.The Astrophysical Journal, 1974
- 2s-2p Transitions in the Spectra of CA XVII and TI XIXThe Astrophysical Journal, 1973
- The Solar Spectrum: Wavelengths and Identifications from 60 TO 385 AngstromsThe Astrophysical Journal, 1972
- Classification of highly ionized emission lines due to transitions from singly and doubly excited levels in sodium, magnesium, aluminium, silicon, phosphorus, sulphur and chlorineJournal of Physics B: Atomic and Molecular Physics, 1970
- The Spectra of Highly Ionized Light Elements in a High Temperature PlasmaProceedings of the Physical Society, 1963