Degree of ionisation of Fe lines in the solar spectrum in the range 170 – 220 Å
- 1 January 1965
- journal article
- Published by Elsevier in Physics Letters
- Vol. 14 (1), 40-41
- https://doi.org/10.1016/0031-9163(65)91043-7
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- A method of differentiating between atomic spectra of high degrees of ionizationJournal of Quantitative Spectroscopy and Radiative Transfer, 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 Spectrum Photographed to 33 .The Astronomical Journal, 1964
- Observations of the Zeta Spectrum in the Wave-length Range 16 Å–400 ÅNature, 1963
- Vacuum Ultraviolet SpectrometerReview of Scientific Instruments, 1963
- Possible Solid-State Effect on the Degree of Ionization Obtained in a Vacuum SparkJournal of Applied Physics, 1962
- A Spectrum of the Sun from 168 to 700 A.The Astronomical Journal, 1962
- Interplanetary Ionization by Solar Extreme Ultraviolet Radiation.The Astrophysical Journal, 1960
- Extreme Ultraviolet Series in Cr VI, Mn VII and Fe VIIIPhysical Review B, 1937