Solar prominences in the extreme ultraviolet as observed from the Apollo Telescope Mount
- 1 March 1974
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 39 (2) , 337-347
- https://doi.org/10.1007/bf00162427
Abstract
No abstract availableKeywords
This publication has 15 references indexed in Scilit:
- Thermal instability of coronal neutral sheets and the formation of quiescent prominencesSolar Physics, 1973
- Analysis of the Extreme-Ultraviolet Quiet Solar SpectrumThe Astrophysical Journal, 1972
- Extreme-Ultraviolet Emission from Solar ProminencesThe Astrophysical Journal, 1972
- The Density Dependent Ionization Balance of Carbon,Oxygen and Neon in the Solar AtmosphereMonthly Notices of the Royal Astronomical Society, 1972
- Energy balance in cool quiescent prominencesSolar Physics, 1971
- Electron densities derived from line intensity ratios: Beryllium isoelectronic sequenceSolar Physics, 1971
- Hydrogen ionization and n=2 population for model spicules and prominencesSolar Physics, 1971
- Spectral analysis of four quiescent prominences observed at the Peruvian eclipseSolar Physics, 1971
- The solar Lyman continuum and the structure of the solar chromosphereSolar Physics, 1970
- On the interpretation of the solar ultraviolet emission line spectrumSpace Science Reviews, 1964