A new method for the analysis of the solar photospheric spectrum |
| |
| Authors: | P. Persi |
| |
| Affiliation: | 1. Laboratorio di Astrofisica Spaziale C.N.R., Frascati, Italy
|
| |
| Abstract: | A new numerical method for the analysis of the high dispersion photospheric spectrum is described. In particular the method is applied to study the C2(0, 0) d 3 Πg-a a Πu molecular band. From measurements of the equivalent widths of C2 lines, a rotational temperature of 4450 ± 305 K is obtained, and the band intensity log W 0 /S 0 = ?0.051 ± 0.101 is found. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
