Hyperfine and Zeeman structure of lines of Bi I

The hyperfine structure (hfs) and Zeeman splitting of 10 lines of Bi I covering the ultraviolet-near-infrared spectral range-359.6, 412.2, 430.9, 449.3, 472.3, 555.2, 613.5, 699.1, 965.7, and 982.8 nm-have been measured. We used a standard spectroscopic technique supported by a sensitive CCD detecti...

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Bibliographic Details
Published in:Journal of the Optical Society of America. B, Optical physics Optical physics, 2014-12, Vol.31 (12), p.3038-3041
Main Authors: Sobolewski, Ł. M., Werbowy, S., Kwela, J.
Format: Article
Language:English
Subjects:
Constants
Covering
Hyperfine structure
Spectral lines
Spectroscopic analysis
Spectroscopy
Splitting
Zeeman effect
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Summary:The hyperfine structure (hfs) and Zeeman splitting of 10 lines of Bi I covering the ultraviolet-near-infrared spectral range-359.6, 412.2, 430.9, 449.3, 472.3, 555.2, 613.5, 699.1, 965.7, and 982.8 nm-have been measured. We used a standard spectroscopic technique supported by a sensitive CCD detection system and precise computer analysis. The Zeeman effect studies were performed for the transverse direction of observation and separated [pi]( Delta M = 0) and [sigma]( Delta M = + or -1) components of lines. The magnetic-dipole (A) hfs constants as well as Lande-g sub(J) factors of Bi I were determined for 10 levels: 32588.22, 41124.99, 42940.52, 43912.37, 44865.08, 45915.88, 49460.91, 50599.67, 55424.3, and 56088.2 cm super(-1).
ISSN:0740-3224
1520-8540
DOI:10.1364/JOSAB.31.003038