On the presence of SH in the sunspot spectrum
โ Scribed by G. C. Joshi; M. C. Pande
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 307 KB
- Volume
- 62
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
The expected equivalent widths of individual rotational lines of the most intense 02 branch of the 0--0 band of the AaX--X2Hi system of $32H and 534H have been calculated in the umbral spectrum for five disk positions using Zwaan's (1974) sunspot model. Percentage abundance of S 34 in the terrestrial case has been considered valid in our calculations.
๐ SIMILAR VOLUMES
Indirect evidence against the presence of C2 lines in umbral spectra is discussed. The dominant role of CO in the molecular equilibrium of C at umbral temperatures ensures that CN, CH and Cz lines are formed in the same atmospheric regions. Observations of CN and CH umbral lines are in good accord w
The equivalent widths of the TiO lines in the a system have been measured on a high dispersion (11 mm/A,) spectrogram of large sunspot. The lines were so weak that the measurement was made by methods giving maximum and minimum equivalent widths, depending on the adopted continuum. The rotational tem