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Q branches in the rotational spectrum of HOClThe far IR rotational spectrum of HOCl from 70-263/cm have been obtained. The most prominent features of the rotational spectrum are the Q branches, for which positions have been measured. Statistical strengths for the Q branches have been calculated and mu sub b, the component of the dipole moment that allows Q branch transitions, has been determined from P and R branch line intensities. It is found that mu sub b = 1.4 + or - 0.2 D. Q branch strengths and shifts at stratospheric temperature are calculated.
Document ID
19830036655
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Chance, K. V.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Traub, W. A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1983
Publication Information
Publication: Journal of Quantitative Spectroscopy and Radiative Transfer
Volume: 29
Subject Category
Atomic And Molecular Physics
Accession Number
83A17873
Funding Number(s)
CONTRACT_GRANT: NSG-5175
Distribution Limits
Public
Copyright
Other

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