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The solar abundance of berylliumThe solar abundance of beryllium is deduced from high-resolution Kitt Peak observations of the 3130.43- and 3131.08-A lines of Be II interpreted by the method of spectrum synthesis. The results are in good agreement with those previously obtained by Grevesse (1968) and by Hauge and Engvold (1968) and indicate that in the photospheric layers, beryllium is depleted below the chondritic value by a factor of about two. It is found that the beryllium abundance is equal to logN(Be)/N(H) + 12 = 1.08 plus or minus 0.05.
Document ID
19740052703
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
74A35453
Funding Number(s)
CONTRACT_GRANT: NGR-05-007-046
Distribution Limits
Public
Copyright
Other

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