Line ratios for solar ultra-violet lines of O v
Abstract
New O V rate coefficients are used to calculate the ratio of the intensity of the 760 Å multiplet to that of the 630 Å line. Results are given for a range of electron densities and temperatures. The theoretical ratios are compared with observed line ratios for different solar regions.
- Publication:
-
Solar Physics
- Pub Date:
- December 1983
- DOI:
- 10.1007/BF00217248
- Bibcode:
- 1983SoPh...89..243D
- Keywords:
-
- Line Spectra;
- Oxygen Spectra;
- Solar Spectra;
- Ultraviolet Astronomy;
- Electron Density (Concentration);
- Electron Impact;
- Plasma Temperature;
- Proton Impact;
- Satellite-Borne Instruments;
- Solar Physics;
- Rate Coefficient;
- Line Ratio;
- Theoretical Ratio;
- Solar Region;
- Observe Line Ratio