Radio and EUV observations of a coronal hole
- 1 May 1977
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 52 (2) , 349-367
- https://doi.org/10.1007/bf00149652
Abstract
No abstract availableKeywords
This publication has 36 references indexed in Scilit:
- A Discussion on the physics of the solar atmosphere - A magnetic model of the solar transition regionPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1976
- Extreme-ultraviolet observations of coronal holes - Initial results from SKYLABThe Astrophysical Journal, 1974
- Models of the Chromospheric-Coronal Transition Layer and Lower Corona Derived from Extreme-Ultraviolet ObservationsThe Astrophysical Journal, 1973
- Analysis of the Extreme-Ultraviolet Quiet Solar SpectrumThe Astrophysical Journal, 1972
- Calculations of Ionization Equilibria for Oxygen, Neon, Silicon, and IronThe Astrophysical Journal, 1969
- Abundance Analyses from Extreme-Ultraviolet Emission LinesThe Astrophysical Journal, 1968
- Theoretical Line Intensities. V. Solar UV Emission Lines of Heavy ElementsThe Astrophysical Journal, 1966
- Excitation of lithium-like ions by electron impactsProceedings of the Physical Society, 1966
- Thermal Diffusion in Ionized GasesProceedings of the Physical Society, 1958
- The derivation of a model solar chromosphere from radio dataProceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, 1950