Bowen, I. S. (1927) Series spectra of boron, carbon, nitrogen, oxygen, and fluorine. Physical Review, 29 (2). pp. 231-247. ISSN 0031-899X http://resolver.caltech.edu/CaltechAUTHORS:BOWpr27a
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Practically all of the unidentified strong lines of boron, carbon, nitrogen, oxygen, and fluorine occurring in the extreme ultra-violet spectra of the vacuum spark have been classified as due to jumps between levels in BI, CI, CII, NII, NIII, OII, OIII, OIV, FI, FII, FIII, and FIV. The levels thus found are correlated with those demanded by the Russell-Heisenberg-Pauli-Hund theory.
|Additional Information:||©1927 The American Physical Society. Received 11 November 1926.|
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|Deposited By:||Tony Diaz|
|Deposited On:||17 Oct 2006|
|Last Modified:||26 Dec 2012 09:05|
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