What is the difference between `emission' and `depression' contribution functions?
Abstract
The right approach to the problem of the depth of Fraunhofer line formation enables us to distinguish the main processes involved in the formation of a Fraunhofer line and to locate the depths for these processes in the photosphere.
- Publication:
-
Solar Physics
- Pub Date:
- December 1991
- DOI:
- 10.1007/BF00146533
- Bibcode:
- 1991SoPh..136..239G
- Keywords:
-
- Absorption Spectra;
- Fraunhofer Lines;
- Photosphere;
- Solar Spectra;
- Emission Spectra;
- Line Spectra;
- Stellar Atmospheres;
- Solar Physics;
- Depression;
- Main Process;
- Line Formation;
- Contribution Function;
- Solar Phenomenon