The browser you are using is not supported by this website. All versions of Internet Explorer are no longer supported, either by us or Microsoft (read more here: https://www.microsoft.com/en-us/microsoft-365/windows/end-of-ie-support).

Please use a modern browser to fully experience our website, such as the newest versions of Edge, Chrome, Firefox or Safari etc.

Paul Miller. Photo.

Paul Miller

Senior lecturer

Paul Miller. Photo.

The EC-Earth3 Earth system model for the Coupled Model Intercomparison Project 6

Author

  • Ralf Döscher
  • Mario Acosta
  • Andrea Alessandri
  • Peter Anthoni
  • Thomas Arsouze
  • Tommi Bergman
  • Raffaele Bernardello
  • Souhail Boussetta
  • Louis Philippe Caron
  • Glenn Carver
  • Miguel Castrillo
  • Franco Catalano
  • Ivana Cvijanovic
  • Paolo Davini
  • Evelien Dekker
  • Francisco J. Doblas-Reyes
  • David Docquier
  • Pablo Echevarria
  • Uwe Fladrich
  • Ramon Fuentes-Franco
  • Matthias Gröger
  • Jost V. Hardenberg
  • Jenny Hieronymus
  • M. Pasha Karami
  • Jukka Pekka Keskinen
  • Torben Koenigk
  • Risto Makkonen
  • François Massonnet
  • Martin Ménégoz
  • Paul A. Miller
  • Eduardo Moreno-Chamarro
  • Lars Nieradzik
  • Twan Van Noije
  • Paul Nolan
  • Declan O'donnell
  • Pirkka Ollinaho
  • Gijs Van Den Oord
  • Pablo Ortega
  • Oriol Tintó Prims
  • Arthur Ramos
  • Thomas Reerink
  • Clement Rousset
  • Yohan Ruprich-Robert
  • Philippe Le Sager
  • Torben Schmith
  • Roland Schrödner
  • Federico Serva
  • Valentina Sicardi
  • Marianne Sloth Madsen
  • Benjamin Smith
  • Tian Tian
  • Etienne Tourigny
  • Petteri Uotila
  • Martin Vancoppenolle
  • Shiyu Wang
  • David Wårlind
  • Ulrika Willén
  • Klaus Wyser
  • Shuting Yang
  • Xavier Yepes-Arbós
  • Qiong Zhang

Summary, in English

The Earth system model EC-Earth3 for contributions to CMIP6 is documented here, with its flexible coupling framework, major model configurations, a methodology for ensuring the simulations are comparable across different high-performance computing (HPC) systems, and with the physical performance of base configurations over the historical period. The variety of possible configurations and sub-models reflects the broad interests in the EC-Earth community. EC-Earth3 key performance metrics demonstrate physical behavior and biases well within the frame known from recent CMIP models. With improved physical and dynamic features, new Earth system model (ESM) components, community tools, and largely improved physical performance compared to the CMIP5 version, EC-Earth3 represents a clear step forward for the only European community ESM. We demonstrate here that EC-Earth3 is suited for a range of tasks in CMIP6 and beyond.

Department/s

  • eSSENCE: The e-Science Collaboration
  • Centre for Environmental and Climate Science (CEC)
  • Dept of Physical Geography and Ecosystem Science
  • BECC: Biodiversity and Ecosystem services in a Changing Climate
  • MERGE: ModElling the Regional and Global Earth system

Publishing year

2022-04-08

Language

English

Pages

2973-3020

Publication/Series

Geoscientific Model Development

Volume

15

Issue

7

Document type

Journal article

Publisher

Copernicus GmbH

Topic

  • Meteorology and Atmospheric Sciences
  • Geosciences, Multidisciplinary

Keywords

  • climate modeling
  • CMIP
  • methodology

Status

Published

ISBN/ISSN/Other

  • ISSN: 1991-959X