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
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
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.