Relative Spektralphotometrie der Sonnenkorona
Abstract
During the total solar eclipse of June 30, 1973, an Austrian expedition in Kenya made the attempt to observe the solar corona with a multiple slit spectrograph. Details concerning the path of the rays in the employed multiple slit spectrograph are considered. The obtained spectra were studied with the aid of a PDS-1000 microdensitometer. A polynomial of the third degree was used in connection with the numerical processing of the corona spectra. A graph is presented showing the relative spectral log E-distribution in the solar corona.
- Publication:
-
Mitteilungen der Astronomischen Gesellschaft Hamburg
- Pub Date:
- 1976
- Bibcode:
- 1976MitAG..40..163L
- Keywords:
-
- Astronomical Photometry;
- Coronagraphs;
- Solar Corona;
- Spectrographs;
- Spectroscopic Analysis;
- Astronomical Spectroscopy;
- Light Scattering;
- Slits;
- Solar Eclipses;
- Solar Physics