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11 IMSC Session Program<br />

Are there lessons for historical climate field reconstruction<br />

from paleoclimatology?<br />

Monday - Plenary Session 4<br />

Michael N. Evans<br />

Dept. of Geology and Earth System Science Interdisciplinary Center, University of<br />

Maryland, College Park, USA<br />

The comparatively severe issues in reconstruction of global gridded climate fields<br />

from high resolution paleoproxy data throw the challenges facing historical<br />

reconstructions based on instrumental data into sharp relief. When observations are<br />

scarce, irregularly distributed in space and/or time, and contain large random errors<br />

and biases, stiff tests for methodological innovations are provided.<br />

In developing observational inputs, we should redouble data archaeological efforts in<br />

underobserved regions, and improve subgrid-scale replication using multiple<br />

measurement systems and data archives. We may need to focus on resolution of the<br />

most energetic syntopic patterns, but avoid reliance on demonstrably unstable<br />

teleconnection patterns. We should also use multiple direct and indirect means to<br />

derive observational uncertainty estimates based on external precision at the grid<br />

scale, and employ the subgridscale distribution of observations in the reconstruction<br />

framework.<br />

At the stage of analysis and infilling of climate fields, we can use efficient joint<br />

spatiotemporal covariance recognition algorithms to identify and exploit tightly<br />

coupled aspects of the climate system. We should employ simple process models as<br />

physical constraints on the results, and data-level models to identify and incorporate<br />

gridscale observational uncertainties into the reconstruction algorithm. As products<br />

we should emphasize the statistical distribution of analyses over central measures as<br />

end products. Finally, we should seek out all possible validation exercises spanning<br />

the satellite, historical and late Holocene eras.<br />

Abstracts 30

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