Abundances in the Solar Corona
Abstract
On the basis of the coronal measurements of the 30 May 1965 eclipse, and using improved atomic parameters, we discuss the coronal abundance determination. Two new line identffications are suggested and several existing suggestions for possible identffications are discussed on the basis of predicted intensities and abundances. Finally an extensive list is given of lines which are possibly observable, together with predicted intensity and equivalent width. Key words: corona - abundances - forbidden line identffications
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- February 1972
- Bibcode:
- 1972A&A....16..417D