MEASUREMENT OF THE ABUNDANCE OF (CO)-C-14 IN THE ATMOSPHERE AND THE C-13 C-12 AND O-18 O-16 RATIO OF ATMOSPHERIC CO WITH APPLICATIONS IN NEW-ZEALAND AND ANTARCTICA

Citation
Cam. Brenninkmeijer, MEASUREMENT OF THE ABUNDANCE OF (CO)-C-14 IN THE ATMOSPHERE AND THE C-13 C-12 AND O-18 O-16 RATIO OF ATMOSPHERIC CO WITH APPLICATIONS IN NEW-ZEALAND AND ANTARCTICA, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 98(D6), 1993, pp. 10595-10614
Citations number
56
Categorie Soggetti
Metereology & Atmospheric Sciences
Volume
98
Issue
D6
Year of publication
1993
Pages
10595 - 10614
Database
ISI
SICI code
Abstract
Equipment and method for accurate and precise concentration, C-14, C-1 3, and O-18 isotope analysis for CO in background air is presented alo ng with new results for Antarctica and New Zealand. High flow rate cry ogenic extraction systems which separate CO after its oxidation to CO2 are used, incorporating a novel ultraefficient cryogenic trap. Air in quantities from a few hundred liters to 2 m3 With CO concentrations f rom 20 part per billion by volume (ppbv) to 1000 ppbv can be analyzed. The absolute CO concentration is determined volumetrically. The C-13/ C-12 and O-18/O-16 ratios are determined by mass spectrometry. For O-1 8 a correction is applied for the oxygen in the CO2 derived from the o xidant. Carbon 14 is determined by accelerator mass spectrometry. Prio r to this the very small CO-derived samples with their high specific a ctivity are diluted accurately. For polluted air the proportional decr ease in specific activity with increasing CO levels is confirmed. The (CO)-C-14 abundance and CO concentration in background air in New Zeal and and Antarctica are not much different, and both follow a distinct seasonal pattern, in particular (CO)-C-14 which is mainly forced by OH seasonality. The (CO)-C-14 abundance swings between its February mini mum of about 6 and its August maximum of about 13 molecules per cm3 ai r (STP). CO has a smaller seasonality and shows a larger scatter due t o local CO sources. The impact of changes in solar activity on (CO)-C- 14 for the period considered has been small. Most of the short-term va riability in (CO)-C-14 is due to the sampling of different air masses. It appears that interannual OH variations may be reflected in (CO)-C- 14 variations. Both C-13/C-12 and O-18/O-16 at Scott Base show large s easonal variation, and the impact of biomass burning and isotopic frac tionation in CO destruction are used to try to explain the respective isotopic compositions.