Sensitivity of the quasi-biennial oscillation to climate change

The period of quasi-biennial oscillation (QBO) of equatorial stratospheric winds is mainly determined by the magnitude of upward momentum transport by equatorial waves and the intensity of the Brewer-Dobson circulation. The observed QBO period is an average of 28 months, but it can range from 24 to...

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Main Author: Doege, M.
Format: Other/Unknown Material
Language:English
Published: University of Hamburg 2003
Subjects:
Online Access:http://hdl.handle.net/11858/00-001M-0000-0012-01F7-6
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spelling ftpubman:oai:pure.mpg.de:item_995358 2023-08-27T04:11:57+02:00 Sensitivity of the quasi-biennial oscillation to climate change Doege, M. 2003 http://hdl.handle.net/11858/00-001M-0000-0012-01F7-6 eng eng University of Hamburg http://hdl.handle.net/11858/00-001M-0000-0012-01F7-6 info:eu-repo/semantics/other 2003 ftpubman 2023-08-02T01:56:14Z The period of quasi-biennial oscillation (QBO) of equatorial stratospheric winds is mainly determined by the magnitude of upward momentum transport by equatorial waves and the intensity of the Brewer-Dobson circulation. The observed QBO period is an average of 28 months, but it can range from 24 to 30 months. The purpose of this study is to find out how sensitive the period and other characteristics of the QBO are to the climate change caused by doubling CO₂ concentration. MAECHAM5 T42L90 experiments are conducted with initial values and boundary conditions (sea ice cover, sea surface temperature) acquired from the AMIP2 climatology and two lower-resolution coupled runs of ECHAM5 and MPI-OM1 with CO₂concentrations of 348 and 696 ppmv, respectively. In a test experiment with unchanged gravity wave parameterization, both a speedup of the Brewer-Dobson circulation and a significant increase in convective precipitation variance observed. Increased variance in the diabatic forcing of the tropical atmosphere leads to strengthened excitation of vertically propagation waves, specifically of gravity waves. Thus two sensitivity experiments with different parameter settings of the subgrid scale gravity wave drag parameterization are analyzed. A speedup of the oscillation from the control experiment value of 34 months to between 22 and 17 minths is observed, where easterly (westerly) phase duration decrease mostly at upper (lower) QBO levels. While the Brewer-Dobson circulation also intensifies due to stronger forcing by the breaking of extratropical planetary waves, it does not offset the enhanced generation of both parameterized and resolved waves. Discrimination between zonal wind forcing by resolved and parameterized waves reveals considerable changes in the parameterized forcing, which extends to lower levels and intensifies, especially maximum westward acceleration. REsolved wave forcing seems to increase mostly between 10 and 20 hPa. Considerable uncertainty about the exact amount of QBO period shorting remains and ... Other/Unknown Material Sea ice Max Planck Society: MPG.PuRe
institution Open Polar
collection Max Planck Society: MPG.PuRe
op_collection_id ftpubman
language English
description The period of quasi-biennial oscillation (QBO) of equatorial stratospheric winds is mainly determined by the magnitude of upward momentum transport by equatorial waves and the intensity of the Brewer-Dobson circulation. The observed QBO period is an average of 28 months, but it can range from 24 to 30 months. The purpose of this study is to find out how sensitive the period and other characteristics of the QBO are to the climate change caused by doubling CO₂ concentration. MAECHAM5 T42L90 experiments are conducted with initial values and boundary conditions (sea ice cover, sea surface temperature) acquired from the AMIP2 climatology and two lower-resolution coupled runs of ECHAM5 and MPI-OM1 with CO₂concentrations of 348 and 696 ppmv, respectively. In a test experiment with unchanged gravity wave parameterization, both a speedup of the Brewer-Dobson circulation and a significant increase in convective precipitation variance observed. Increased variance in the diabatic forcing of the tropical atmosphere leads to strengthened excitation of vertically propagation waves, specifically of gravity waves. Thus two sensitivity experiments with different parameter settings of the subgrid scale gravity wave drag parameterization are analyzed. A speedup of the oscillation from the control experiment value of 34 months to between 22 and 17 minths is observed, where easterly (westerly) phase duration decrease mostly at upper (lower) QBO levels. While the Brewer-Dobson circulation also intensifies due to stronger forcing by the breaking of extratropical planetary waves, it does not offset the enhanced generation of both parameterized and resolved waves. Discrimination between zonal wind forcing by resolved and parameterized waves reveals considerable changes in the parameterized forcing, which extends to lower levels and intensifies, especially maximum westward acceleration. REsolved wave forcing seems to increase mostly between 10 and 20 hPa. Considerable uncertainty about the exact amount of QBO period shorting remains and ...
format Other/Unknown Material
author Doege, M.
spellingShingle Doege, M.
Sensitivity of the quasi-biennial oscillation to climate change
author_facet Doege, M.
author_sort Doege, M.
title Sensitivity of the quasi-biennial oscillation to climate change
title_short Sensitivity of the quasi-biennial oscillation to climate change
title_full Sensitivity of the quasi-biennial oscillation to climate change
title_fullStr Sensitivity of the quasi-biennial oscillation to climate change
title_full_unstemmed Sensitivity of the quasi-biennial oscillation to climate change
title_sort sensitivity of the quasi-biennial oscillation to climate change
publisher University of Hamburg
publishDate 2003
url http://hdl.handle.net/11858/00-001M-0000-0012-01F7-6
genre Sea ice
genre_facet Sea ice
op_relation http://hdl.handle.net/11858/00-001M-0000-0012-01F7-6
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