Determination of the temperature of the solar corona from the spectrum of the electron-scattering continuum
- 1 May 1976
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 48 (1) , 3-19
- https://doi.org/10.1007/bf00153327
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Comment on the paper ?Two-Fluid Model of the Solar Corona? by J. W. Knight, C. E. Newman, and P. A. SturrockSolar Physics, 1975
- The profile and polarization of the coronal L? lineSolar Physics, 1974
- Analysis of the Extreme-Ultraviolet Quiet Solar SpectrumThe Astrophysical Journal, 1972
- Magnetic fields and the structure of the solar coronaSolar Physics, 1970
- On the Obliteration of Strong Fraunhofer Lines by Electron Scattering in the Solar CoronaPublications of the Astronomical Society of the Pacific, 1968
- The Ionization Equilibrium for Iron in the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1964
- Polarization and Intensity Studies of the Eclipse of October 2, 1959.The Astrophysical Journal, 1961
- A New Instrument for Observing the Electron Corona.The Astrophysical Journal, 1957
- “Turbulence”, kinetic temperature, and electron temperature in stellar atmospheresVistas in Astronomy, 1955
- The Doppler Effect in Resonance LinesProceedings of the National Academy of Sciences, 1940