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Timeslice environment3/17/2023 We consider 10 different solutions between 3.6 and 5.0 Ma alongside the Lisiecki and Raymo (2004) and Ahn et al (2017) benthic oxygen isotope records and the record of magnetic reversals (Gradstein et al (2020)). As derived from the astronomical solution (Laskar et al 2004), we use the annual insolation pattern at the top of the atmosphere to determine which time slices have the most similar to modern orbital configuration. To this end, we show plausible time slices during the Early Pliocene that have similar to modern orbital forcing. This time slice became the key target for the second Pliocene Modelling Intercomparison Project (PlioMIP2) and data reconstructions led by the USGS PRISM Group and the PAGES PlioVAR group.Īs part of the planning for PlioMIP3, the community is considering whether a simulation in the Early Pliocene (5.3 – 3.6 Ma) would be a useful target for modelling groups. It occurred during a period of orbital forcing that was very similar to present day. This time slice centred on 3.205 Ma (3.204–3.207 Ma) is a warm interval characterized by a negative benthic oxygen isotope excursion (0.21–0.23‰) centred on marine isotope stage KM5c (KM5.3). Haywood et al (2013) identified a time slice within the Piacenzian that presented a target for modellers and the data community for reconstructing a mid-Pliocene climate and environment. In part this uncertainty was due to the proxy reconstructions being based on a time slab (of ~300,000 years). Uncertainties in the prescribed climate model forcings and in proxy data were shown to limit our ability to truly evaluate the models. Following the first Pliocene Model Intercomparison Project (PlioMIP), data-model comparisons showed that regionally there were significant discrepancies between predictions of climate.
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