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U.S. Department of Energy
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Photochemical modeling of the earth's stratosphere

Thesis/Dissertation ·
OSTI ID:6218773
A one-dimensional photochemical model of the Earth's stratosphere has been developed in order to provide an up-to-date comparison with mid-latitude observations. The first-order effects of the inclusion of the diffuse radiation in a spherical shell atmosphere, for solar zenith angles close to 90/sup 0/ are demonstrated. Changes in model concentrations are largest for short-lived radicals such as O, OH, ClO, and NO in the lower stratosphere, but relatively small compared to current observational uncertainties. It is proposed that a significant overestimate of the molecular oxygen absorption cross section near 210 nm is in large part responsible for the discrepancy between observed and modeled vertical profiles of some halocarbons (CFCl/sub 3/ in particular). The diurnal variation of ClO observed from the ground by P. Solomon and coworkers is consistent with these diurnal model results and provides indirect evidence for the existence of ClONO/sub 2/. The main uncertainty relating to fluorine products concerns the value of the quantum yield for COF/sub 2/ photodissociation. The mean observed mid-latitude ozone abundance from about 35 to 50 km is up to 60% greater than current model results. Given the uncertainties in laboratory photochemical data, it is difficult to reconcile theory and observations; the model chemistry might be missing a significant ingredient. Certain observations of a daytime increase in ozone near 40 km are also puzzling. Fast isotopic exchange reactions between O and O/sub 2/ dominate the heavy ozone photochemistry, so that a large enhancement in heavy ozone cannot be sustained in the stratosphere, contrary to the observations of K. Mauersberger.
OSTI ID:
6218773
Country of Publication:
United States
Language:
English