The abundance of chlorine in the Sun
β Scribed by D. L. Lambert; E. A. Mallia
- Publisher
- Springer
- Year
- 1968
- Tongue
- English
- Weight
- 273 KB
- Volume
- 5
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
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.
π SIMILAR VOLUMES
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
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βThe emotions flying between the two women who tell their story here is as dramatic as the Appalachian Trail and as tumultuous as the Atlantic Ocean. These natural elements are a perfect backdrop for the revelations of love which both repel and engage them.β β Jewelle Gomez, author, _The Gilda Stori