- 1University of East Anglia, Centre for Ocean and Atmospheric Sciences, School of Environmental Sciences, Norwich, United Kingdom of Great Britain and Northern Ireland (kaiser2@gmail.com)
- 2National Centre for Atmospheric Science, University of East Anglia, Norwich, United Kingdom of Great Britain and Northern Ireland
- 3Aerodyne Research, Billerica, Massachusetts, United States of America
During the AMT31 research cruise (Southampton–Montevideo, December 2024), we measured CO2 polyisotopologues using a tuneable infrared laser direct absorption spectrometer (Aerodyne TILDAS-FD-L2). Dried marine air from an inlet at the bow of the ship was alternated with a working reference every 2 min to correct for instrument drift.
Compared with land-based measurements, ship motion (roll, pitch, heave) was found to deteriorate isotope ratio precision by a factor of 3 to 10 (depending on the sea state). However, after averaging over hourly intervals, precisions better than 0.05 µmol mol–1 for y(CO2) and better than 0.03 ‰ for δ(13C), δ(18O) and δ(17O) were achieved. For the 17O isotope excess, Δ(17O), hourly precision was often better than 10 ppm (0.01 ‰), but unfortunately, target tank results showed unexplained day-to-day variability of the order of ±35 ppm.
Preliminary corrections for this day-to-day variability indicate that southern hemisphere δ(18O) is 1.2–1.8 ‰ higher and Δ(17O) is about 60 ppm higher than northern hemisphere marine background air. This interhemispheric Δ(17O) gradient is twice as high as predicted by atmosphere-biosphere exchange models (Koren et al., 2019) and could indicate a stronger than expected influence of the 17O-enriched stratospheric return flux in austral spring or a stronger biospheric exchange signal in boreal autumn.
How to cite: Kaiser, J., Pickers, P. A., Forster, G. L., Marca, A., Paxton, R. B., and McManus, B.: Atlantic Meridional Transect of polyisotopic carbon dioxide: Challenges of ship-based laser spectroscopy and implications for atmosphere-biosphere exchange, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13314, https://doi.org/10.5194/egusphere-egu25-13314, 2025.