Non-LTE profiles of strong solar lines
Abstract
The complete linearization method is applied to the formation of strong lines in the solar atmosphere. Transitions in Na(I), Mg(I), Ca(I), Mg(II), and Ca(II) are computed with a standard atmosphere and microturbulent velocity model. The computed profiles are compared to observations at disk center.
- Publication:
-
Contributions of the Observatory of New Mexico State University, Las Cruces Special Series
- Pub Date:
- April 1976
- Bibcode:
- 1976CONMS...1..110S
- Keywords:
-
- Atmospheric Models;
- Line Spectra;
- Solar Atmosphere;
- Calcium;
- Linearization;
- Magnesium;
- Sodium;
- Temperature Profiles;
- Transition Temperature;
- Turbulence;
- Solar Physics