Positionally dependent 15N fractionation factors in the UV photolysis of N2O determined by high resolution FTIR spectroscopy

被引：37

作者：

Turatti, F ^{[1
]}

Griffith, DWT

Wilson, SR

Esler, MB

Rahn, T

Zhang, H

Blake, GA

机构：

[1] Univ Wollongong, Dept Chem, Wollongong, NSW 2522, Australia

[2] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA

来源：

GEOPHYSICAL RESEARCH LETTERS | 2000年 / 27卷 / 16期

关键词：

D O I：

10.1029/2000GL011371

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Positionally dependent fractionation factors for the photolysis of isotopomers of N2O in natural abundance have been determined by high resolution FTIR spectroscopy at three photolysis wavelengths. Fractionation factors show clear N-15 position and photolysis wavelength dependence and are in qualitative agreement with theoretical models but are twice as large. The fractionation factors increase with photolysis wavelength from 193 to 211 nm, with the fractionation factors at 207.6 nm for (NNO)-N-14-N-15-O-16, (NNO)-N-15-N-14-O-16 and (NNO)-N-14-N-14-O-18 equal to -66.5 +/- 5 parts per thousand -27.1 +/- 6 parts per thousand and -49 +/- 10 parts per thousand, respectively.

引用

页码：2489 / 2492

页数：4