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The solar abundance of thuliumConsideration of one relatively unblended line of the solar spectrum, namely, the 3131.258-A line of Tm II, which yields a thulium abundance of 0.80 plus or minus 0.10 with the Corliss and Bozman (1962) f-value. The uncertainty of this figure is discussed in conjunction with the contradictory findings of some other investigators. The need for further detailed study of the lanthanides by the method of spectrum synthesis is pointed out.
Document ID
19740052704
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ross, J. E.
Aller, L. H.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
May 1, 1974
Publication Information
Publication: Solar Physics
Volume: 36
Subject Category
Space Sciences
Accession Number
74A35454
Funding Number(s)
CONTRACT_GRANT: NGL-05-007-046
Distribution Limits
Public
Copyright
Other

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