๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Abundance of Helium in the Sun

โœ Scribed by LAMBERT, D. L.


Book ID
109657220
Publisher
Nature Publishing Group
Year
1967
Tongue
English
Weight
258 KB
Volume
215
Category
Article
ISSN
0028-0836

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Abundance of Boron in the Sun
โœ LAMBERT, D. L.; MALLIA, E. A.; WARNER, B. ๐Ÿ“‚ Article ๐Ÿ“… 1966 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 191 KB
Helium abundance in Novae
โœ I. Malakpour ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 186 KB
The abundance of chlorine in the Sun
โœ D. L. Lambert; E. A. Mallia ๐Ÿ“‚ Article ๐Ÿ“… 1968 ๐Ÿ› Springer ๐ŸŒ English โš– 273 KB

The Cll line 2 8375.943 (4s aPs:,., 9 4p-."D%:,.) is identified in the solar spectrum. This is the tirst identification of a chlorine line in solar spectrum. The measured equivalent width (W;. --0.8 rnJk) corresponds to an abttndance IogN(Cl)-5.65 on the scale [ogN(H).. ]2.00.

Helium abundance in the solar wind
โœ K. W. Ogilvie; T. D. Wilkerson ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 852 KB
Abundances of heavy elements in the sun
โœ Nicolas Grevesse ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 777 KB

Solar abundances have been derived for Pb, Bi, Th and U. For the three lirst elements, the abundances are determined from the profiles of their lines obtained with the high resolution solar spectrometer installed at the Jungfraujoch Scientific Station (Switzerland) and fi'om new oscillator strengths