Statistical regularities in the solar spectrum
Abstract
The paper examines the dependence of halfwidth and equivalent width for Fe I lines on their excitation potential observed in the solar spectrum (Babiia, 1988). It is shown that the dependence can be explained within the framework of the modern theory of the formation of spectral lines.
- Publication:
-
Pisma v Astronomicheskii Zhurnal
- Pub Date:
- March 1990
- Bibcode:
- 1990PAZh...16..260K
- Keywords:
-
- Solar Atmosphere;
- Solar Spectra;
- Spectral Line Width;
- Fraunhofer Lines;
- Iron;
- Statistical Analysis;
- Solar Physics