Coronal abundance of elements and a model of the quiet Sun from radio observations
- 1 October 1972
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 26 (2), 343-353
- https://doi.org/10.1007/bf00165275
Abstract
No abstract availableKeywords
This publication has 25 references indexed in Scilit:
- The Extreme-Ultraviolet Spectrum of the Quiet SunThe Astrophysical Journal, 1971
- Theoretical Line Intensities. V. Solar UV Emission Lines of Heavy ElementsThe Astrophysical Journal, 1966
- Solar Observations at 3.2 MM.The Astrophysical Journal, 1965
- On the interpretation of the solar ultraviolet emission line spectrumSpace Science Reviews, 1964
- Symposium on Radar and Radiometric Observations of Venus during the 1962 Conjunction: Observations of Venus, the Sun, Moon, and Tau A at 1.18-cm wavelengthThe Astronomical Journal, 1964
- Solar Emission at Millimeter Wave Lengths.The Astrophysical Journal, 1961
- "Imferon"BMJ, 1960
- The Distribution of Radio Brightness over the Solar Disk at a Wavelength of 21 Centimetres. III. The Quiet Sun ? Two-Dimensional ObservationsAustralian Journal of Physics, 1955
- Brightness of the Solar Disk at a Wave Length of 10.3 Centimeters.The Astrophysical Journal, 1954
- Temperature Gradient in the Sun's Atmosphere Measured at Radio Frequencies.The Astrophysical Journal, 1951