The abundance of chlorine in the Sun |
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| Authors: | D L Lambert E A Mallia |
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| Institution: | (1) Dept. of Astrophysics, University Observatory, Oxford;(2) Present address: Mount Wilson and Palomar Observatories, Pasadena, Calif., U.S.A. |
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| Abstract: | The Cli line  8375.943 (4s 4P5/2 – 4p 4D 7/2) is identified in the solar spectrum. This is the first identification of a chlorine line in solar spectrum. The measured equivalent width (W
= 0.8 mÅ) corresponds to an abundance log N(Cl) = 5.65 on the scale log N(H) = 12.00. |
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