A Born-Oppenheimer photolysis model of N2O fractionation -: art. no. 1656

被引:30
作者
Blake, GA [1 ]
Liang, MC [1 ]
Morgan, CG [1 ]
Yung, YL [1 ]
机构
[1] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
关键词
D O I
10.1029/2003GL016932
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The isotopically light N2O produced by microbial activity is thought to be balanced by the return of heavy stratospheric nitrous oxide. The Yung and Miller [1997] method that first explained these trends yields photolytic fractionation factors similar tohalf those observed by experiment or predicted quantum mechanically, however. To address these issues, we present here a Born-Oppenheimer photolysis model that uses only commonly available spectroscopic data. The predicted fractionations quantitatively reproduce laboratory data, and have been incorporated into zonally averaged atmospheric simulations. Like McLinden et al. [2003], who employ a three-dimensional chemical transport model with cross sections scaled to match laboratory data, we find excellent agreement between predictions and stratospheric measurements; additional processes that contribute to the mass independent anomaly in N2O can only account for a fraction of its global budget.
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页数:4
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