Classification of Iron Lines in the Spectrum of the Sun and Zeta in the Range 167 Å to 220 Å
- 1 April 1965
- journal article
- Published by Springer Nature in Nature
- Vol. 206 (4982), 390-392
- https://doi.org/10.1038/206390a0
Abstract
No abstract availableThis publication has 7 references indexed in Scilit:
- New Spectra of the Iron Transition Elements of Astrophysical Interest.The Astrophysical Journal, 1965
- Degree of ionisation of Fe lines in the solar spectrum in the range 170 – 220 ÅPhysics Letters, 1965
- Identification of Extreme Ultraviolet Solar Emission Lines.The Astrophysical Journal, 1964
- Comparison of Solar and Laboratory Iron Spectra in the Vacuum Ultraviolet.The Astrophysical Journal, 1964
- Origin of Certain Solar Emission Lines Between 170 and 220 Å.The Astrophysical Journal, 1964
- Solar Xuv-Spectrum from 310 Å to 55 Å.The Astrophysical Journal, 1964
- Observations of the Zeta Spectrum in the Wave-length Range 16 Å–400 ÅNature, 1963