$^{39}$Ar dating with small samples resolves ocean ventilation
Ocean ventilation is the integrated effect of various processes that propagate surface properties to the ocean interior. Its precise understanding is the prerequisite for addressing essential questions such as oxygen supply, the storage of anthropogenic carbon and the heat budget of the ocean. Curre...
| Main Authors: | , , , , , , , , |
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| Format: | Report |
| Language: | unknown |
| Published: |
arXiv
2018
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| Subjects: | |
| Online Access: | https://dx.doi.org/10.48550/arxiv.1807.11146 https://arxiv.org/abs/1807.11146 |
| Summary: | Ocean ventilation is the integrated effect of various processes that propagate surface properties to the ocean interior. Its precise understanding is the prerequisite for addressing essential questions such as oxygen supply, the storage of anthropogenic carbon and the heat budget of the ocean. Currently employed observational methods to infer ventilation utilise transient tracers, i.e. tritium, SF$_6$, CFCs and the radioisotope $^{14}$C. However, their dating ranges are not suitable to resolve the dynamics of the deep ocean. The noble gas isotope $^{39}$Ar with a half-life of 269 years fills this gap. Its broad application has previously been hindered by its very low abundance, requiring at least 1000 litres of water for dating. Here we report on successful $^{39}$Ar dating with only 5 litres of water based on the atom-optical technique Atom Trap Trace Analysis. Our data reveal previously not quantifiable ventilation patterns in the Eastern Tropical North Atlantic, where we find that advection is more important for the ventilation of the intermediate depth range than previously assumed. This result implies faster ventilation than estimated in other studies and thus a significantly higher anthropogenic CO$_2$-storage. The demonstrated analytical capabilities now allow for a global collection of $^{39}$Ar data, which will have significant impact on our understanding of ocean ventilation. |
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