Development of a probabilistic ocean modelling system based on NEMO 3.5: application at eddying resolution

This paper presents the technical implementation of a new, probabilistic version of the NEMO ocean–sea-ice modelling system. Ensemble simulations with N members running simultaneously within a single executable, and interacting mutually if needed, are made possible through an enhanced message-passin...

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Bibliographic Details
Published in:Geoscientific Model Development
Main Authors: Bessières, Laurent, Leroux, Stéphanie, Brankart, Jean-Michel, Molines, Jean-Marc, Moine, Marie-Pierre, Bouttier, Pierre-Antoine, Penduff, Thierry, Terray, Laurent, Barnier, Bernard, Sérazin, Guillaume
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/gmd-10-1091-2017
https://gmd.copernicus.org/articles/10/1091/2017/
Description
Summary:This paper presents the technical implementation of a new, probabilistic version of the NEMO ocean–sea-ice modelling system. Ensemble simulations with N members running simultaneously within a single executable, and interacting mutually if needed, are made possible through an enhanced message-passing interface (MPI) strategy including a double parallelization in the spatial and ensemble dimensions. An example application is then given to illustrate the implementation, performances, and potential use of this novel probabilistic modelling tool. A large ensemble of 50 global ocean–sea-ice hindcasts has been performed over the period 1960–2015 at eddy-permitting resolution (1∕4°) for the OCCIPUT (oceanic chaos – impacts, structure, predictability) project. This application aims to simultaneously simulate the intrinsic/chaotic and the atmospherically forced contributions to the ocean variability, from mesoscale turbulence to interannual-to-multidecadal timescales. Such an ensemble indeed provides a unique way to disentangle and study both contributions, as the forced variability may be estimated through the ensemble mean, and the intrinsic chaotic variability may be estimated through the ensemble spread.