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    ENSO Diabatic Heating in ECMWF and NCEP–NCAR Reanalyses, and NCAR CCM3 Simulation

    Source: Journal of Climate:;2000:;volume( 013 ):;issue: 017::page 3152
    Author:
    Nigam, Sumant
    ,
    Chung, Chul
    ,
    DeWeaver, Eric
    DOI: 10.1175/1520-0442(2000)013<3152:EDHIEA>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Diabatic heating associated with El Niño?Southern Oscillation (ENSO) variability is residually diagnosed from the European Centre for Medium-Range Forecasts (ECMWF) and National Centers for Environmental Prediction (NCEP)?National Center for Atmospheric Research (NCAR) atmospheric reanalysis datasets during the overlapping 1979?93 period. Quantitative characterization of the horizontal and vertical structure of ENSO heating anomalies, including estimates of uncertainty, provides observationally constrained validation targets for GCM physical parameterizations. The diagnosed ENSO heating anomalies have similar horizontal structure, but the vertically averaged ECMWF heating is stronger and in better agreement with the Xie?Arkin precipitation anomalies, particularly with respect to precipitation reduction over the western tropical Pacific. Comparison of heating vertical structures in the central equatorial Pacific shows ECMWF heating to be considerably stronger in the lower troposphere, where it exhibits a local maximum. The ENSO covariant tropospheric temperature in the two reanalyses was also examined along the equator and found to have an intriguing vertical structure, with sizeable amplitude in the lower and upper troposphere and vanishing amplitude in between. The largest temperature anomalies in the lower troposphere are at the surface, and the ECMWF one is about 50% stronger. The three-dimensional heating anomalies diagnosed from the reanalyses are used to evaluate the ENSO heating distribution produced by NCAR?s Community Climate Model, version 3 (CCM3) atmospheric GCM, when integrated in a climate simulation mode. At least, in context of ENSO variability, the differences in ECMWF and NCEP heating anomalies are small in comparison with CCM3?s heating departures from either of these anomalies, allowing characterization of the CCM3?s ENSO heating structure: horizontally, as a more meridional redistribution (?Hadley-like?), and vertically, as a substantially ?bottom-heavy? profile, relative to the reanalyses anomalies. In a companion paper, deficiencies in the simulated ENSO surface winds are related to specific features of the CCM3?s heating error, from diagnostic modeling.
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      ENSO Diabatic Heating in ECMWF and NCEP–NCAR Reanalyses, and NCAR CCM3 Simulation

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    contributor authorNigam, Sumant
    contributor authorChung, Chul
    contributor authorDeWeaver, Eric
    date accessioned2017-06-09T15:52:20Z
    date available2017-06-09T15:52:20Z
    date copyright2000/09/01
    date issued2000
    identifier issn0894-8755
    identifier otherams-5558.pdf
    identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4195711
    description abstractDiabatic heating associated with El Niño?Southern Oscillation (ENSO) variability is residually diagnosed from the European Centre for Medium-Range Forecasts (ECMWF) and National Centers for Environmental Prediction (NCEP)?National Center for Atmospheric Research (NCAR) atmospheric reanalysis datasets during the overlapping 1979?93 period. Quantitative characterization of the horizontal and vertical structure of ENSO heating anomalies, including estimates of uncertainty, provides observationally constrained validation targets for GCM physical parameterizations. The diagnosed ENSO heating anomalies have similar horizontal structure, but the vertically averaged ECMWF heating is stronger and in better agreement with the Xie?Arkin precipitation anomalies, particularly with respect to precipitation reduction over the western tropical Pacific. Comparison of heating vertical structures in the central equatorial Pacific shows ECMWF heating to be considerably stronger in the lower troposphere, where it exhibits a local maximum. The ENSO covariant tropospheric temperature in the two reanalyses was also examined along the equator and found to have an intriguing vertical structure, with sizeable amplitude in the lower and upper troposphere and vanishing amplitude in between. The largest temperature anomalies in the lower troposphere are at the surface, and the ECMWF one is about 50% stronger. The three-dimensional heating anomalies diagnosed from the reanalyses are used to evaluate the ENSO heating distribution produced by NCAR?s Community Climate Model, version 3 (CCM3) atmospheric GCM, when integrated in a climate simulation mode. At least, in context of ENSO variability, the differences in ECMWF and NCEP heating anomalies are small in comparison with CCM3?s heating departures from either of these anomalies, allowing characterization of the CCM3?s ENSO heating structure: horizontally, as a more meridional redistribution (?Hadley-like?), and vertically, as a substantially ?bottom-heavy? profile, relative to the reanalyses anomalies. In a companion paper, deficiencies in the simulated ENSO surface winds are related to specific features of the CCM3?s heating error, from diagnostic modeling.
    publisherAmerican Meteorological Society
    titleENSO Diabatic Heating in ECMWF and NCEP–NCAR Reanalyses, and NCAR CCM3 Simulation
    typeJournal Paper
    journal volume13
    journal issue17
    journal titleJournal of Climate
    identifier doi10.1175/1520-0442(2000)013<3152:EDHIEA>2.0.CO;2
    journal fristpage3152
    journal lastpage3171
    treeJournal of Climate:;2000:;volume( 013 ):;issue: 017
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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