Predicted wavelengths of coronal transitions in the configurations 3s 23p 2, 3s 23p 3 and 3s 23p 4
- 1 June 1971
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 18 (2) , 232-243
- https://doi.org/10.1007/bf00145936
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Analyses of the XUV Spectra of K, Ca, Sc and Ti Isoelectronic with P I, Si I and Al IPhysica Scripta, 1970
- The solar limb emission spectrum between 300 Å and 2803 ÅSolar Physics, 1970
- On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal linesSolar Physics, 1969
- Redetermined Level Values and Interaction Parameters of S i and Cl ii Ground ConfigurationsJournal of the Optical Society of America, 1969
- Vacuum Ultraviolet Wavelength Standards and Improved Energy Levels in the First Spectrum of Silicon*Journal of the Optical Society of America, 1967
- The Ultraviolet Emission Spectrum of the Solar Chromosphere and CoronaMonthly Notices of the Royal Astronomical Society, 1967
- Wave Lengths of Forbidden Nebular Lines. IIThe Astrophysical Journal, 1960
- Atomic Energy Levels and Spectra of Neutral and Singly Ionized Phosphorus (P i and P ii)*†Journal of the Optical Society of America, 1959