High n Emission and Absorption Lines of the Sun (II)
Abstract
Considering the electronic pressure broadening of highn solar recombination lines, an upper wavelength limit of the observable region of possible lines is derived. The reason that no lines have been observed is discussed.
- Publication:
-
Solar Physics
- Pub Date:
- February 1975
- DOI:
- 10.1007/BF00162379
- Bibcode:
- 1975SoPh...40..329G
- Keywords:
-
- Absorption Spectra;
- Emission Spectra;
- Pressure Broadening;
- Solar Spectra;
- Spectral Line Width;
- Line Spectra;
- Optical Transition;
- Recombination Reactions;
- Solar Magnetic Field;
- Spectroheliographs;
- Zeeman Effect;
- Solar Physics;
- Recombination;
- Absorption Line;
- Recombination Line;
- Wavelength Limit;
- Electronic Pressure