Full text

Turn on search term navigation

Copyright Copernicus GmbH 2011

Abstract

The isotopic composition of volatile organic compounds (VOCs) can provide valuable information on their sources and fate not deducible from mixing ratios alone. In particular the reported carbon stable isotope ratios of chloromethane and bromomethane from different sources cover a δ13 C-range of almost 100[per thousand] making isotope ratios a very promising tool for studying the biogeochemistry of these compounds. So far, the determination of the isotopic composition of C1 and C2 halocarbons others than chloromethane is hampered by their low mixing ratios.

In order to determine the carbon isotopic composition of C1 and C2 halocarbons with mixing ratios as low as 1 pptv (i) a field suitable cryogenic high volume sampling system and (ii) a chromatographic set up for processing these samples have been developed and validated. The sampling system was tested at two different sampling sites, an urban and a coastal location in Northern Germany. The average δ13 C-values for bromomethane at the urban site were -42.9 ± 1.1[per thousand] and agreed well with previously published results. But at the coastal site bromomethane was substantially enriched in 13 C by almost 10[per thousand]. Less pronounced differences were observed for chlorodifluoromethane, 1,1,1-trichloroethane and chloromethane. We suggest that these differences are related to the turnover of these compounds in ocean surface waters. Furthermore we report first carbon isotope ratios for iodomethane (-40.4[per thousand] to -79.8[per thousand]), bromoform (-13.8[per thousand] to 22.9[per thousand]), and other halocarbons.

Details

Title
A high volume sampling system for isotope determination of volatile halocarbons and hydrocarbons
Author
Bahlmann, E.; Weinberg, I.; Seifert, R.; Tubbesing, C.; Michaelis, W.
First page
2073
Publication year
2011
Publication date
2011
Publisher
Copernicus GmbH
ISSN
18671381
e-ISSN
18678548
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
1010616499
Copyright
Copyright Copernicus GmbH 2011