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Equatorial Kelvin wave signatures in ozone profile measurements from Global Ozone Monitoring Experiment (GOME)

Identifieur interne : 000212 ( PascalFrancis/Curation ); précédent : 000211; suivant : 000213

Equatorial Kelvin wave signatures in ozone profile measurements from Global Ozone Monitoring Experiment (GOME)

Auteurs : R. M. A. Timmermans [Pays-Bas] ; R. F. Van Oss [Pays-Bas] ; H. M. Kelder [Pays-Bas]

Source :

RBID : Pascal:06-0065634

Descripteurs français

English descriptors

Abstract

This study investigates the ability to derive height-resolved information on equatorial Kelvin wave activity from three different Global Ozone Monitoring Experiment (GOME) ozone profile data sets. The ozone profiles derived using the Ozone Profile Retrieval Algorithm (OPERA) based on optimal estimation and the Neural Network Ozone Retrieval System (NNORSY) both show Kelvin wave signals in agreement with previously identified signals in the GOME total ozone columns. However, because of the inadequate vertical resolution, these two data sets are not able to resolve the vertical structure of the Kelvin wave activity. The third data set, consisting of assimilated OPERA ozone profiles, does provide height-resolved information on Kelvin wave activity that is consistent with results from the analysis of GOME total ozone columns and ECMWF Re-Analysis (ERA-40) temperature data. Largest Kelvin-wave-induced perturbations of up to 0.69 DU/km coincide with the maximum vertical gradient in ozone around 35 hPa and show an in-phase relationship with temperature perturbations in ERA-40 as expected from theoretical considerations. These results indicate that the ozone perturbations in the lower stratosphere and in the total column of ozone are transport related. Between 10 and 1 hPa, large Kelvin-wave-induced fluctuations in ozone mixing ratio are present that, however, because of their small contribution to the total column, do not constitute a large contribution to the total ozone column perturbations. The ozone perturbations between 10 and 1 hPa show an out-of-phase relationship with temperature perturbations in ERA-40, indicating that the perturbations can either be caused by transport effects or photochemical influences.
pA  
A01 01  1    @0 0148-0227
A03   1    @0 J. geophys. res.
A05       @2 110
A06       @2 D21
A08 01  1  ENG  @1 Equatorial Kelvin wave signatures in ozone profile measurements from Global Ozone Monitoring Experiment (GOME)
A11 01  1    @1 TIMMERMANS (R. M. A.)
A11 02  1    @1 VAN OSS (R. F.)
A11 03  1    @1 KELDER (H. M.)
A14 01      @1 Royal Netherlands Meteorological Institute @2 De Bilt @3 NLD @Z 1 aut. @Z 2 aut. @Z 3 aut.
A20       @2 D21103.1-D21103.15
A21       @1 2005
A23 01      @0 ENG
A43 01      @1 INIST @2 3144 @5 354000134564890030
A44       @0 0000 @1 © 2006 INIST-CNRS. All rights reserved.
A45       @0 27 ref.
A47 01  1    @0 06-0065634
A60       @1 P
A61       @0 A
A64 01  1    @0 Journal of geophysical research
A66 01      @0 USA
C01 01    ENG  @0 This study investigates the ability to derive height-resolved information on equatorial Kelvin wave activity from three different Global Ozone Monitoring Experiment (GOME) ozone profile data sets. The ozone profiles derived using the Ozone Profile Retrieval Algorithm (OPERA) based on optimal estimation and the Neural Network Ozone Retrieval System (NNORSY) both show Kelvin wave signals in agreement with previously identified signals in the GOME total ozone columns. However, because of the inadequate vertical resolution, these two data sets are not able to resolve the vertical structure of the Kelvin wave activity. The third data set, consisting of assimilated OPERA ozone profiles, does provide height-resolved information on Kelvin wave activity that is consistent with results from the analysis of GOME total ozone columns and ECMWF Re-Analysis (ERA-40) temperature data. Largest Kelvin-wave-induced perturbations of up to 0.69 DU/km coincide with the maximum vertical gradient in ozone around 35 hPa and show an in-phase relationship with temperature perturbations in ERA-40 as expected from theoretical considerations. These results indicate that the ozone perturbations in the lower stratosphere and in the total column of ozone are transport related. Between 10 and 1 hPa, large Kelvin-wave-induced fluctuations in ozone mixing ratio are present that, however, because of their small contribution to the total column, do not constitute a large contribution to the total ozone column perturbations. The ozone perturbations between 10 and 1 hPa show an out-of-phase relationship with temperature perturbations in ERA-40, indicating that the perturbations can either be caused by transport effects or photochemical influences.
C02 01  2    @0 220
C02 02  3    @0 001E
C02 03  2    @0 001E01
C03 01  X  FRE  @0 Onde Kelvin @5 01
C03 01  X  ENG  @0 Kelvin wave @5 01
C03 01  X  SPA  @0 Onda Kelvin @5 01
C03 02  2  FRE  @0 Ozone @5 02
C03 02  2  ENG  @0 ozone @5 02
C03 02  2  SPA  @0 Ozono @5 02
C03 03  2  FRE  @0 Monde @5 03
C03 03  2  ENG  @0 global @5 03
C03 03  2  SPA  @0 Mundo @5 03
C03 04  2  FRE  @0 Surveillance @5 04
C03 04  2  ENG  @0 monitoring @5 04
C03 04  2  SPA  @0 Vigilancia @5 04
C03 05  2  FRE  @0 Etude expérimentale @5 05
C03 05  2  ENG  @0 experimental studies @5 05
C03 06  X  FRE  @0 Hauteur @5 06
C03 06  X  ENG  @0 Height @5 06
C03 06  X  SPA  @0 Altura @5 06
C03 07  X  FRE  @0 Estimation optimale @5 07
C03 07  X  ENG  @0 Optimal estimation @5 07
C03 07  X  SPA  @0 Estimación óptima @5 07
C03 08  2  FRE  @0 Réseau neuronal @5 08
C03 08  2  ENG  @0 neural networks @5 08
C03 08  2  SPA  @0 Red neuronal @5 08
C03 09  X  FRE  @0 Contenu total ozone @5 09
C03 09  X  ENG  @0 Total ozone content @5 09
C03 09  X  SPA  @0 Contenido total ozono @5 09
C03 10  2  FRE  @0 Température @5 10
C03 10  2  ENG  @0 temperature @5 10
C03 10  2  SPA  @0 Temperatura @5 10
C03 11  X  FRE  @0 Perturbation @5 11
C03 11  X  ENG  @0 Perturbation @5 11
C03 11  X  SPA  @0 Perturbación @5 11
C03 12  X  FRE  @0 Gradient vertical @5 12
C03 12  X  ENG  @0 Vertical gradient @5 12
C03 12  X  SPA  @0 Gradiente vertical @5 12
C03 13  2  FRE  @0 Stratosphère @5 13
C03 13  2  ENG  @0 stratosphere @5 13
C03 13  2  SPA  @0 Estratosfera @5 13
C03 14  2  FRE  @0 Transport @5 14
C03 14  2  ENG  @0 transport @5 14
C03 14  2  SPA  @0 Transporte @5 14
C03 15  2  FRE  @0 Fluctuation @5 15
C03 15  2  ENG  @0 fluctuations @5 15
C03 15  2  SPA  @0 Fluctuación @5 15
C03 16  X  FRE  @0 Rapport mélange @5 16
C03 16  X  ENG  @0 Mixing ratio @5 16
C03 16  X  SPA  @0 Relación mezcla @5 16
N21       @1 037
N44 01      @1 OTO
N82       @1 OTO

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Pascal:06-0065634

Le document en format XML

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<div type="abstract" xml:lang="en">This study investigates the ability to derive height-resolved information on equatorial Kelvin wave activity from three different Global Ozone Monitoring Experiment (GOME) ozone profile data sets. The ozone profiles derived using the Ozone Profile Retrieval Algorithm (OPERA) based on optimal estimation and the Neural Network Ozone Retrieval System (NNORSY) both show Kelvin wave signals in agreement with previously identified signals in the GOME total ozone columns. However, because of the inadequate vertical resolution, these two data sets are not able to resolve the vertical structure of the Kelvin wave activity. The third data set, consisting of assimilated OPERA ozone profiles, does provide height-resolved information on Kelvin wave activity that is consistent with results from the analysis of GOME total ozone columns and ECMWF Re-Analysis (ERA-40) temperature data. Largest Kelvin-wave-induced perturbations of up to 0.69 DU/km coincide with the maximum vertical gradient in ozone around 35 hPa and show an in-phase relationship with temperature perturbations in ERA-40 as expected from theoretical considerations. These results indicate that the ozone perturbations in the lower stratosphere and in the total column of ozone are transport related. Between 10 and 1 hPa, large Kelvin-wave-induced fluctuations in ozone mixing ratio are present that, however, because of their small contribution to the total column, do not constitute a large contribution to the total ozone column perturbations. The ozone perturbations between 10 and 1 hPa show an out-of-phase relationship with temperature perturbations in ERA-40, indicating that the perturbations can either be caused by transport effects or photochemical influences.</div>
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<s5>13</s5>
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<fC03 i1="13" i2="2" l="SPA">
<s0>Estratosfera</s0>
<s5>13</s5>
</fC03>
<fC03 i1="14" i2="2" l="FRE">
<s0>Transport</s0>
<s5>14</s5>
</fC03>
<fC03 i1="14" i2="2" l="ENG">
<s0>transport</s0>
<s5>14</s5>
</fC03>
<fC03 i1="14" i2="2" l="SPA">
<s0>Transporte</s0>
<s5>14</s5>
</fC03>
<fC03 i1="15" i2="2" l="FRE">
<s0>Fluctuation</s0>
<s5>15</s5>
</fC03>
<fC03 i1="15" i2="2" l="ENG">
<s0>fluctuations</s0>
<s5>15</s5>
</fC03>
<fC03 i1="15" i2="2" l="SPA">
<s0>Fluctuación</s0>
<s5>15</s5>
</fC03>
<fC03 i1="16" i2="X" l="FRE">
<s0>Rapport mélange</s0>
<s5>16</s5>
</fC03>
<fC03 i1="16" i2="X" l="ENG">
<s0>Mixing ratio</s0>
<s5>16</s5>
</fC03>
<fC03 i1="16" i2="X" l="SPA">
<s0>Relación mezcla</s0>
<s5>16</s5>
</fC03>
<fN21>
<s1>037</s1>
</fN21>
<fN44 i1="01">
<s1>OTO</s1>
</fN44>
<fN82>
<s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
</record>

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