EGU24-3596, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-3596
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Measuring δ17O and Δ′17O in precipitation across various spatial and temporal scales: spanning from global to local and from multi-year to sub-hourly resolutions

Stefan Terzer-Wassmuth1, Luis Araguas-Araguas1, Leonard I. Wassenaar1,2, Lucilena R. Monteiro3,1, and Christine Stumpp4
Stefan Terzer-Wassmuth et al.
  • 1International Atomic Energy Agency, NAPC/Isotope Hydrology Section, Vienna, Austria (s.terzer@iaea.org)
  • 2WasserCluster Lunz Biologische Station GmbH, Lunz am See, Austria
  • 3Instituto de Pesquisas Energéticas e Nucleares, IPEN/CNEN, São Paulo, SP, Brazil.
  • 4Department of Water, Atmosphere and Environment, Institute of Soil Physics and Rural Water Management, University of Natural Resources and Life Sciences, Vienna, Austria

During the past decade, the rare O isotope 17O and the 17O-excess became attractive for potential new applications in hydrology, climatology, and broader oxygen isotope research. Although laser-based analysers are technologically capable of the needed Δ′17O assays, progress was hindered by the metrological challenges and the absence of fundamental spatiotemporal data on precipitation inputs. Uncertainties surrounding the input function of the water cycle complicate advancements of 17O as a tracer. This “emerging tracer dilemma” is a potential obstacle for further triple-O isotope research.

In this work, >3500 archived water samples from the Global Network of Precipitation (GNIP) sample archives (2015-2021) were re-analysed for  for δ17O and Δ′17O. For >60 GNIP stations, four or more years’ of samples were analysed, assessing the seasonality of Δ′17O, and constructing δ17O/ δ18O Local Meteoric Water Lines (LMWL). This global dataset allowed for a first-ever comprehensive assessment of the spatial patterns of δ17O/ δ18O LMWLs, and to devise a first-ever precipitation-weighted Global Meteoric Water Line (GMWL): δ′17O = 0.5280 ± 0.0002 δ′18O + 0.0153 ± 0.0013. This GMWL definition is similar to previous efforts albeit with a lower ordinate intercept.

We further analysed the Δ′17O of a 6-year daily/fortnightly precipitation sampling in Vienna as an example of seasonal isotopic variations at synoptic weather patterns’ resolution. Air moisture sources were determined by backwards trajectory analysis and corroborated with synoptic weather data from Austria’s meteorological service. The Δ′17O values correlated with δ18O seasonality. A comparison with the deuterium excess patterns (stemming from the Atlantic and Mediterranean domains) demonstrated that the “two excesses” carried different signals. While elevated d-excesses
mainly came from the central/eastern Mediterranean Sea or easterly continental sources during all seasons, we found elevated Δ′17O precipitation originated only from northerly or north-easterly sources, and predominantly during the winter season.

Finally, we present pilot Vienna precipitation events sampled at sub-hourly (to 5-minute) resolution, which included both cyclonic and convective rainfall events, which demonstrate the interplay of moisture sources using triple oxygen isotopes and deuterium excess. This work will help to shape our understanding of δ17O and Δ′17O in Earth’s precipitation, despite the ongoing metrological challenges faced, and promote discussion regarding the scientific value of routine measurements for triple-oxygen isotopes in precipitation.

How to cite: Terzer-Wassmuth, S., Araguas-Araguas, L., Wassenaar, L. I., Monteiro, L. R., and Stumpp, C.: Measuring δ17O and Δ′17O in precipitation across various spatial and temporal scales: spanning from global to local and from multi-year to sub-hourly resolutions, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-3596, https://doi.org/10.5194/egusphere-egu24-3596, 2024.