Models of Thermodynamic Properties of Prominences.
Abstract
The thermodynamic properties of solar prominences are considered insofar as they relate to the energetics and mass transport of the latter. The present emphasis is on obtaining accurate indicators of electron temperature, electron energy and thickness from the line and recombination emission spectra of prominences. Some proposals for future work in this field are presented.
- Publication:
-
IAU Colloq. 44: Physics of Solar Prominences
- Pub Date:
- 1979
- Bibcode:
- 1979phsp.coll..349M
- Keywords:
-
- Mass Transfer;
- Solar Prominences;
- Solar Spectra;
- Thermodynamic Properties;
- Abundance;
- Emission Spectra;
- H Lines;
- Helium;
- Line Spectra;
- Lyman Spectra;
- Solar Physics