Abstract
Tropical and midlatitude precipitation is fundamentally of two types, spatially limited and high-intensity convective or widespread and lower-intensity stratiform, owing to differences in vertical air motions and microphysical processes governing rain formation. These processes are difficult to observe or model and precipitation partitioning into rain types is critical for understanding how the water cycle responds to changes in climate. Here, we combine two independent data sets—convective and stratiform precipitation fractions, derived from the Tropical Rainfall Measuring Mission satellite or synoptic cloud observations, and stable isotope and tritium compositions of surface precipitation, derived from a global network—to show that isotope ratios reflect rain type proportions and are negatively correlated with stratiform fractions. Condensation and riming associated with boundary layer moisture produces higher isotope ratios in convective rain, along with higher tritium when riming in deep convection occurs with entrained air at higher altitudes. On the basis of our data, stable isotope ratios can be used to monitor changes in the character of precipitation in response to periodic variability or changes in climate. Our results also provide observational constraints for an improved simulation of convection in climate models and a better understanding of isotope variations in proxy archives, such as speleothems and tropical ice.
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Acknowledgements
We thank E. Izewski of IAEA for assistance with graphic illustrations.
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P.K.A. initiated the project and wrote the paper; U.R., D.B., C.S. and A.F. provided TRMM data; L.A.-A. processed isotope and related data; P.B. contributed cloud-based stratiform fractions; all authors contributed to data evaluation and commented on the manuscript.
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Aggarwal, P., Romatschke, U., Araguas-Araguas, L. et al. Proportions of convective and stratiform precipitation revealed in water isotope ratios. Nature Geosci 9, 624–629 (2016). https://doi.org/10.1038/ngeo2739
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DOI: https://doi.org/10.1038/ngeo2739
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