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Polynomial coefficients for calculating O2 Schumann-Runge cross sections at 0.5/cm resolutionO2 cross sections from 49,000 to 57,000/cm have been fitted with temperature dependent polynomial expressions, providing an accurate and efficient means of determining Schumann-Runge band cross sections for temperatures between 130 and 500 K. The least squares fits were carried out on a 0.5/cm spectral grid, using cross sections obtained from a Schumann-Runge line-by-line model that incorporates the most recent spectroscopic data. The O2 cross sections do not include the underlying Herzberg continuum, but they do contain contributions from the temperature dependent Schumann-Runge continuum. The cross sections are suitable for use in UV transmission calculations at high spectral resolution. They should also prove useful for updating existing parameterizations of ultraviolet transmission and O2 photolysis.
Document ID
19920063176
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Minschwaner, K.
(Harvard University Cambridge, MA, United States)
Anderson, G. P.
(NASA Headquarters Washington, DC United States)
Hall, L. A.
(USAF, Phillips Laboratory, Hanscom AFB MA, United States)
Yoshino, K.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 15, 2013
Publication Date
June 20, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: D9 J
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
92A45800
Funding Number(s)
CONTRACT_GRANT: NSF ATM-83-18960
CONTRACT_GRANT: NSF ATM-89-21119
CONTRACT_GRANT: NAGW-1230
CONTRACT_GRANT: F19628-89-C-0091
Distribution Limits
Public
Copyright
Other

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