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The microwave and far-infrared spectra of the O-(18)H radicalFar-infrared laser magnetic resonance (LMR) spectroscopy was used to calculate the frequencies, wavelengths, and line strengths for transitions of O-(18)H molecules at microwave and far-infrared frequencies. In this experiment, a molecular transition frequency is tuned into coincidence with that of a fixed frequency laser by the application of a variable magnetic field. The O-(18)H radicals, detected in natural abundance (0.20 percent), were produced by the reaction of hydrogen atoms with nitrogen dioxide. These data together with microwave frequencies ascertained by Gottlieb, Redford, and Smith (1974) were used to determine the parameters of an effective Hamiltonian. Rotational levels up to J = 5.5 were involved. Results are indicated schematically and the low-lying energy levels of O-(18)H are shown. It is concluded that the frequencies of transitions between levels studied directly in the LMR experiment are reliable.
Document ID
19860055354
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Comben, E. R.
(Oxford Univ. Oxford, United Kingdom)
Brown, J. M.
(Oxford University United Kingdom)
Steimle, T. C.
(Arizona State University Tempe, United States)
Leopold, K. R.
(Oxford Univ. Oxford, United Kingdom)
Evenson, K. M.
(NBS Boulder, CO, United States)
Date Acquired
August 12, 2013
Publication Date
June 1, 1986
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 305
ISSN: 0004-637X
Subject Category
Inorganic And Physical Chemistry
Accession Number
86A40092
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-15047
Distribution Limits
Public
Copyright
Other

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