๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The possible existence of HOH lines in the sunspot spectrum

โœ Scribed by E. A. Mallia; D. E. Blackwell

Publisher
Springer
Year
1970
Tongue
English
Weight
150 KB
Volume
12
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

The possible presence of C2lines in suns
The possible presence of C2lines in sunspot spectra
โœ D. L. Lambert; E. A. Mallia ๐Ÿ“‚ Article ๐Ÿ“… 1973 ๐Ÿ› Springer ๐ŸŒ English โš– 216 KB

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

On the presence of SH in the sunspot spe
On the presence of SH in the sunspot spectrum
โœ G. C. Joshi; M. C. Pande ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 307 KB

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 terrestria

A study of the green TiO band in the sun
A study of the green TiO band in the sunspot spectrum
โœ Mitsugu Makita ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 542 KB

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