Isotopic Fractionation of Stratospheric Nitrous Oxide

Author:

Yung Yuk L.12,Miller Charles E.12

Affiliation:

1. Y. L. Yung, Division of Geological and Planetary Sciences, California Institute of Technology, Mail Stop 150-21, Pasadena, CA 91125, USA.

2. C. L. Miller, Atmospheric Kinetics and Photochemistry Group, Jet Propulsion Laboratory, California Institute of Technology, Mail Stop 183-901, 4800 Oak Grove Drive, Pasadena, CA 91109–8099, USA.

Abstract

We propose an isotopic fractionation mechanism, based on photolytic destruction, to explain the 15 N/ 14 N and 18 O/ 16 O fractionation of stratospheric nitrous oxide (N 2 O) and reconcile laboratory experiments with atmospheric observations. The theory predicts that (i) the isotopomers 15 N 14 N 16 O and 14 N 15 N 16 O have very different isotopic fractionations in the stratosphere, and (ii) laboratory photolysis experiments conducted at 205 nanometers should better simulate the observed isotopic fractionation of stratospheric N 2 O. Modeling results indicate that there is no compelling reason to invoke a significant chemical source of N 2 O in the middle atmosphere and that individual N 2 O isotopomers might be useful tracers of stratospheric air parcel motion.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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