Rotation of the solar photosphere from observations of central depthsof Fraunhofer lines.
Abstract
The solar rotation velocity for different heliographic latitudes has been found from comparison of the central depths of Fraunhofer lines in the spectrum of the sun as a star with the central depths of the same lines at different distances from the solar centre.
- Publication:
-
Kinematika i Fizika Nebesnykh Tel
- Pub Date:
- December 1985
- Bibcode:
- 1985KFNT....1R..53G
- Keywords:
-
- Fraunhofer Lines;
- Photosphere;
- Solar Atmosphere;
- Solar Rotation;
- Solar Spectra;
- Angular Velocity;
- Spectral Resolution;
- Solar Physics;
- Rotation:Solar Photosphere;
- Solar Photosphere:Rotation