The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses

International audience We compare the tropical oscillations and planetary scale Kelvin waves in four troposphere-stratosphere climate models and the assimilated dataset produced by the United Kingdom Meteorological Office (UKMO). The comparison has been made in the GRIPS framework "GCM-Reality...

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Main Authors: Amodei, M., Pawson, S., Scaife, A. A., Langematz, U., Lahoz, W., Li, D. M., Simon, P.
Other Authors: Centre national de recherches météorologiques (CNRM), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS), Data Assimilation Office, NASA Goddard Space Flight Center (GSFC), Universities Space Research Association Washington (USRA), The Meteorological Office, Freie Universität Berlin, Center for Global Atmospheric Modelling
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2001
Subjects:
Online Access:https://hal.science/hal-00329151
https://hal.science/hal-00329151/document
https://hal.science/hal-00329151/file/angeo-19-99-2001.pdf
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institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Amodei, M.
Pawson, S.
Scaife, A. A.
Langematz, U.
Lahoz, W.
Li, D. M.
Simon, P.
The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
topic_facet [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description International audience We compare the tropical oscillations and planetary scale Kelvin waves in four troposphere-stratosphere climate models and the assimilated dataset produced by the United Kingdom Meteorological Office (UKMO). The comparison has been made in the GRIPS framework "GCM-Reality Intercomparison Project for SPARC", where SPARC is Stratospheric Processes and their Role in Climate, a project of the World Climate Research Program. The four models evaluated are European members of GRIPS: the UKMO Unified Model (UM), the model of the Free University in Berlin (FUB–GCM), the ARPEGE-climat model of the French National Centre for Meteorological Research (CNRM), and the Extended UGAMP GCM (EUGCM) of the Centre for Global Atmospheric Modelling (CGAM). The integrations were performed with different, but annually periodic external conditions (e.g., sea-surface temperature, sea ice, and incoming solar radiation). The structure of the tropical winds and the strengths of the Kelvin waves are examined. In the analyses where the SAO (Semi-Annual Oscillation) and the QBO (Quasi-Biennal Oscillation) are reasonably well captured, the amplitude of these analysed Kelvin waves is close to that observed in independent data from UARS (Upper Atmosphere Research Satellite). In agreement with observations, the Kelvin waves generated in the models propagate into the middle atmosphere as wave packets, consistent with a convective forcing origin. In three of the models, slow Kelvin waves propagate too high and their amplitudes are overestimated in the upper stratosphere and in the mesosphere, the exception is the UM which has weaker waves. None of the modelled waves are sufficient to force realistic eastward phases of the QBO or SAO. Although the SAO is represented by all models, only two of them are able to generate westerlies between 10 hPa and 50 hPa. The importance of the role played in the SAO by unresolved gravity waves is emphasized. Although it exhibits some unrealistic features, the EUGCM, which includes a ...
author2 Centre national de recherches météorologiques (CNRM)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
Data Assimilation Office
NASA Goddard Space Flight Center (GSFC)
Universities Space Research Association Washington (USRA)
The Meteorological Office
Freie Universität Berlin
Center for Global Atmospheric Modelling
format Article in Journal/Newspaper
author Amodei, M.
Pawson, S.
Scaife, A. A.
Langematz, U.
Lahoz, W.
Li, D. M.
Simon, P.
author_facet Amodei, M.
Pawson, S.
Scaife, A. A.
Langematz, U.
Lahoz, W.
Li, D. M.
Simon, P.
author_sort Amodei, M.
title The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
title_short The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
title_full The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
title_fullStr The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
title_full_unstemmed The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses
title_sort sao and kelvin waves in the eurogrips gcms and the uk met. office analyses
publisher HAL CCSD
publishDate 2001
url https://hal.science/hal-00329151
https://hal.science/hal-00329151/document
https://hal.science/hal-00329151/file/angeo-19-99-2001.pdf
genre Sea ice
genre_facet Sea ice
op_source ISSN: 0992-7689
EISSN: 1432-0576
Annales Geophysicae
https://hal.science/hal-00329151
Annales Geophysicae, 2001, 19 (1), pp.99-114
op_relation hal-00329151
https://hal.science/hal-00329151
https://hal.science/hal-00329151/document
https://hal.science/hal-00329151/file/angeo-19-99-2001.pdf
op_rights info:eu-repo/semantics/OpenAccess
_version_ 1789972984317870080
spelling ftinsu:oai:HAL:hal-00329151v1 2024-02-04T10:04:29+01:00 The SAO and Kelvin waves in the EuroGRIPS GCMS and the UK Met. Office analyses Amodei, M. Pawson, S. Scaife, A. A. Langematz, U. Lahoz, W. Li, D. M. Simon, P. Centre national de recherches météorologiques (CNRM) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Data Assimilation Office NASA Goddard Space Flight Center (GSFC) Universities Space Research Association Washington (USRA) The Meteorological Office Freie Universität Berlin Center for Global Atmospheric Modelling 2001 https://hal.science/hal-00329151 https://hal.science/hal-00329151/document https://hal.science/hal-00329151/file/angeo-19-99-2001.pdf en eng HAL CCSD European Geosciences Union hal-00329151 https://hal.science/hal-00329151 https://hal.science/hal-00329151/document https://hal.science/hal-00329151/file/angeo-19-99-2001.pdf info:eu-repo/semantics/OpenAccess ISSN: 0992-7689 EISSN: 1432-0576 Annales Geophysicae https://hal.science/hal-00329151 Annales Geophysicae, 2001, 19 (1), pp.99-114 [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/article Journal articles 2001 ftinsu 2024-01-10T17:25:36Z International audience We compare the tropical oscillations and planetary scale Kelvin waves in four troposphere-stratosphere climate models and the assimilated dataset produced by the United Kingdom Meteorological Office (UKMO). The comparison has been made in the GRIPS framework "GCM-Reality Intercomparison Project for SPARC", where SPARC is Stratospheric Processes and their Role in Climate, a project of the World Climate Research Program. The four models evaluated are European members of GRIPS: the UKMO Unified Model (UM), the model of the Free University in Berlin (FUB–GCM), the ARPEGE-climat model of the French National Centre for Meteorological Research (CNRM), and the Extended UGAMP GCM (EUGCM) of the Centre for Global Atmospheric Modelling (CGAM). The integrations were performed with different, but annually periodic external conditions (e.g., sea-surface temperature, sea ice, and incoming solar radiation). The structure of the tropical winds and the strengths of the Kelvin waves are examined. In the analyses where the SAO (Semi-Annual Oscillation) and the QBO (Quasi-Biennal Oscillation) are reasonably well captured, the amplitude of these analysed Kelvin waves is close to that observed in independent data from UARS (Upper Atmosphere Research Satellite). In agreement with observations, the Kelvin waves generated in the models propagate into the middle atmosphere as wave packets, consistent with a convective forcing origin. In three of the models, slow Kelvin waves propagate too high and their amplitudes are overestimated in the upper stratosphere and in the mesosphere, the exception is the UM which has weaker waves. None of the modelled waves are sufficient to force realistic eastward phases of the QBO or SAO. Although the SAO is represented by all models, only two of them are able to generate westerlies between 10 hPa and 50 hPa. The importance of the role played in the SAO by unresolved gravity waves is emphasized. Although it exhibits some unrealistic features, the EUGCM, which includes a ... Article in Journal/Newspaper Sea ice Institut national des sciences de l'Univers: HAL-INSU