Towards high-resolution climate reconstruction using an off-line data assimilation and COSMO-CLM 5.00 model
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Published:2018-09-24
Issue:9
Volume:14
Page:1345-1360
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ISSN:1814-9332
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Container-title:Climate of the Past
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language:en
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Short-container-title:Clim. Past
Author:
Fallah BijanORCID, Russo Emmanuele, Acevedo Walter, Mauri Achille, Becker NicoORCID, Cubasch Ulrich
Abstract
Abstract. Data assimilation (DA) methods have been used recently to constrain the
climate model forecasts by paleo-proxy records. Both DA and climate models
are computationally very expensive. Moreover, in paleo-DA, the time step of
consequence for observations is usually too long for a dynamical model to
follow the previous analysis state and the chaotic behavior of the model
becomes dominant. The majority of recent paleoclimate studies using DA have
performed low- or intermediate-resolution global simulations along with an
“off-line” DA approach. In an off-line DA, the re-initialization cycle is
completely removed after the assimilation step. In this paper, we design a
computationally affordable DA to assimilate yearly pseudo-observations and
real observations into an ensemble of COSMO-CLM high-resolution regional
climate model (RCM) simulations over Europe, for which the ensemble members
slightly differ in boundary and initial conditions. Within a perfect model
experiment, the performance of the applied DA scheme is evaluated with
respect to its sensitivity to the noise levels of pseudo-observations. It was
observed that the injected bias in the pseudo-observations linearly impacts
the DA skill. Such experiments can serve as a tool for the selection of proxy
records, which can potentially reduce the state estimation error when they
are assimilated. Additionally, the sensitivity of COSMO-CLM to the boundary
conditions is addressed. The geographical regions where the model exhibits
high internal variability are identified. Two sets of experiments are
conducted by averaging the observations over summer and winter. Furthermore,
the effect of the spurious correlations within the observation space is
studied and a optimal correlation radius, within which the observations are
assumed to be correlated, is detected. Finally, the pollen-based
reconstructed quantities at the mid-Holocene are assimilated into the RCM and
the performance is evaluated against a test dataset. We conclude that the DA
approach is a promising tool for creating high-resolution yearly analysis
quantities. The affordable DA method can be applied to efficiently improve
climate field reconstruction efforts by combining high-resolution
paleoclimate simulations and the available proxy records.
Publisher
Copernicus GmbH
Subject
Paleontology,Stratigraphy,Global and Planetary Change
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