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contributor authorHodyss, Daniel
contributor authorCampbell, William F.
contributor authorWhitaker, Jeffrey S.
date accessioned2017-06-09T17:33:31Z
date available2017-06-09T17:33:31Z
date copyright2016/07/01
date issued2016
identifier issn0027-0644
identifier otherams-87189.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4230830
description abstractnsemble-based Kalman filter (EBKF) algorithms are known to produce posterior ensembles whose variance is incorrect for a variety of reasons (e.g., nonlinearity and sampling error). It is shown here that the presence of sampling error implies that the true posterior error variance is a function of the latest observation, as opposed to the standard EBKF, whose posterior variance is independent of observations. In addition, it is shown that the traditional ensemble validation tool known as the ?binned spread-skill? diagram does not correctly identify this issue in the ensemble generation step of the EBKF, leading to an overly optimistic impression of the relationship between posterior variance and squared error. An updated ensemble validation tool is described that reveals the incorrect relationship between mean squared error (MSE) and ensemble variance, and gives an unbiased evaluation of the posterior variances from EBKF algorithms. Last, a new inflation method is derived that accounts for sampling error and correctly yields posterior error variances that depend on the latest observation. The new method has very little computational overhead, does not require access to the observations, and is simple to use in any serial or global EBKF.
publisherAmerican Meteorological Society
titleObservation-Dependent Posterior Inflation for the Ensemble Kalman Filter
typeJournal Paper
journal volume144
journal issue7
journal titleMonthly Weather Review
identifier doi10.1175/MWR-D-15-0329.1
journal fristpage2667
journal lastpage2684
treeMonthly Weather Review:;2016:;volume( 144 ):;issue: 007
contenttypeFulltext


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