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Microwave Observations and Modeling of O2 (1-delta(sub g)) and O3 Diurnal Variation in the MesosphereThe first microwave measurements of an electronically excited molecular species in the Earth's atmosphere are presented. Local thermodynamic equilibrium (LTE) rotational line emission from mesospheric O2(1-del(sub g)) was observed at a frequency of 255.01794 GHz (lambda is approx. 1.2 mm), employing the National Radio Astronomy Observatory (NRAO) millimeter facility at Kitt Peak, Arizona (32 N, 111 W). The pressure broadened line shapes of the O2(1-del(sub g)) spectra, which were obtained in January and April 1992 and in January and November 1993, are inverted to retrieve O2(1-del(sub g)) mixing profiles over the 50-70 km altitude region. The observed daytime abundances exceed ozone abundances in the lower mesosphere, which are separately retrieved with coincident O3 spectral line (249.7886 GHz) observations. The January and November 1993 observations are binned into 20-60 min time intervals to study O2(1-del(sub g)) diurnal behavior. Derived abundances of O2(1-del(sub g)) between 50 and 70 km for the four observation dates are 9%, 31%, 3%, and 26%, respectively, each +/- 10% higher than predicted, based on the simple photochemistry of lower mesospheric O2(1-del(sub g)). Modeled variation of [O2(1-del(sub g))] with time of day agrees with observed variation in that the observed difference between model and data abundances is constant throughout the daylight hours of each observation date. Model underprediction Of [02(lAg)] is consistent with similar model underprediction of mesospheric [O3]. A perturbation to the photochemical model that forces decreased ozone chemical loss brings brings both model [O3] and [O2(1-del(sub g))] into agreement with the observations. O2(1-del(sub g)) abundances derived from these 1.2 mm observations agree with [O2(1-del(sub g))] values derived from comparable SME observations of the 1.27 micrometers emission, with assumption of a 3880 sec O2(1-del(sub g)) radiative lifetime. The 6800 sec O2(1-del(sub g)) radiative lifetime proposed by Mlynczak and Nesbitt is ruled out by the similar comparison.
Document ID
20010058914
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Sandor, Brad J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Clancy, R. Todd
(Space Science Inst. Boulder, CO United States)
Rusch, David W.
(Colorado Univ. Boulder, CO United States)
Randall, Cora E.
(Colorado Univ. Boulder, CO United States)
Eckman, Richard S.
(NASA Langley Research Center Hampton, VA United States)
Siskind, David S.
(Naval Research Lab. Washington, DC United States)
Muhleman, Duane O.
(California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 20, 2013
Publication Date
April 20, 1997
Publication Information
Publication: Journal of Geophysical Research
Publisher: American Geophysical Union
Volume: 102
Issue: D7
ISSN: 0148-0227
Subject Category
Geophysics
Report/Patent Number
Paper-96JD03585
Funding Number(s)
CONTRACT_GRANT: NSF ATM-95-01288
Distribution Limits
Public
Copyright
Other

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