OperaV1, PascalFrancis, Curation, bibRecord, 000315

Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2

Identifieur interne : 000315 ( PascalFrancis/Curation ); précédent : 000314; suivant : 000316

Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2

Auteurs : J. C. A. Van Peet [Pays-Bas] ; R. J. Van Der A [Pays-Bas] ; A. T. J. De Laat [Pays-Bas] ; O. N. E. Tuinder [Pays-Bas] ; G. König-Langlo [Allemagne] ; J. Wittig [Allemagne]

Source :

Geophysical research letters [ 0094-8276 ] ; 2009.

RBID : Pascal:09-0316779

Descripteurs français

Pascal (Inist)
- Hauteur, Trou ozone, Monde, Ozone, Surveillance, Etude expérimentale, Algorithme extraction, Répartition verticale, Stratosphère, Spectre, Longueur onde, Instrumentation, Cycle, Structure 3 dimensions, Tourbillon, Moyenne latitude, Antarctique.
Wicri :
- topic : Ozone.

English descriptors

KwdEn :
- Antarctica, Height, Mid latitude, Ozone holes, Retrieval algorithm, Three dimensional structure, Vertical distribution, Vortex, cycles, experimental studies, global, instruments, monitoring, ozone, spectra, stratosphere, wavelength.

Abstract

We present Global Ozone Monitoring Experiment-2 (GOME-2) ozone profiles that were operationally retrieved with the KNMI Ozone ProfilE Retrieval Algorithm (OPERA) algorithm for the period September-December 2008. It is shown that it is possible to accurately measure the vertical distribution of stratospheric ozone for Antarctic ozone hole conditions from spectra measured at ultraviolet wavelengths from a nadir viewing instrument. Comparisons with ozone sonde observations from the Neumayer station at the Antarctic coast show a good agreement for various ozone profile shapes representing different phases of the annual recurring ozone hole cycle. A preliminary analysis of the three-dimensional structure of the ozone hole shows for example that at the vortex edges ozone rich mid-latitude middle and upper stratospheric layers can be found over ozone depleted lower stratospheric 'ozone hole' layers. These Antarctic ozone profile observations combined with the daily global coverage of GOME-2 enables the monitoring of the three-dimensional structure of the ozone hole on a daily basis.

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A08	`01`	`1`	`ENG`	`@1 Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2`
A11	`01`	`1`		`@1 VAN PEET (J. C. A.)`
A11	`02`	`1`		`@1 VAN DER A (R. J.)`
A11	`03`	`1`		`@1 DE LAAT (A. T. J.)`
A11	`04`	`1`		`@1 TUINDER (O. N. E.)`
A11	`05`	`1`		`@1 KÖNIG-LANGLO (G.)`
A11	`06`	`1`		`@1 WITTIG (J.)`
A14	`01`			`@1 Royal Netherlands Meteorological Institute @2 De Bilt @3 NLD @Z 1 aut. @Z 2 aut. @Z 3 aut. @Z 4 aut.`
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C01	`01`		`ENG`	@0 We present Global Ozone Monitoring Experiment-2 (GOME-2) ozone profiles that were operationally retrieved with the KNMI Ozone ProfilE Retrieval Algorithm (OPERA) algorithm for the period September-December 2008. It is shown that it is possible to accurately measure the vertical distribution of stratospheric ozone for Antarctic ozone hole conditions from spectra measured at ultraviolet wavelengths from a nadir viewing instrument. Comparisons with ozone sonde observations from the Neumayer station at the Antarctic coast show a good agreement for various ozone profile shapes representing different phases of the annual recurring ozone hole cycle. A preliminary analysis of the three-dimensional structure of the ozone hole shows for example that at the vortex edges ozone rich mid-latitude middle and upper stratospheric layers can be found over ozone depleted lower stratospheric 'ozone hole' layers. These Antarctic ozone profile observations combined with the daily global coverage of GOME-2 enables the monitoring of the three-dimensional structure of the ozone hole on a daily basis.
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C03	`07`	`X`	`ENG`	`@0 Retrieval algorithm @5 07`
C03	`07`	`X`	`SPA`	`@0 Algoritmo extracción @5 07`
C03	`08`	`X`	`FRE`	`@0 Répartition verticale @5 08`
C03	`08`	`X`	`ENG`	`@0 Vertical distribution @5 08`
C03	`08`	`X`	`SPA`	`@0 Distribución vertical @5 08`
C03	`09`	`2`	`FRE`	`@0 Stratosphère @5 09`
C03	`09`	`2`	`ENG`	`@0 stratosphere @5 09`
C03	`09`	`2`	`SPA`	`@0 Estratosfera @5 09`
C03	`10`	`2`	`FRE`	`@0 Spectre @5 10`
C03	`10`	`2`	`ENG`	`@0 spectra @5 10`
C03	`10`	`2`	`SPA`	`@0 Espectro @5 10`
C03	`11`	`2`	`FRE`	`@0 Longueur onde @5 11`
C03	`11`	`2`	`ENG`	`@0 wavelength @5 11`
C03	`12`	`2`	`FRE`	`@0 Instrumentation @5 12`
C03	`12`	`2`	`ENG`	`@0 instruments @5 12`
C03	`12`	`2`	`SPA`	`@0 Instrumentación @5 12`
C03	`13`	`2`	`FRE`	`@0 Cycle @5 13`
C03	`13`	`2`	`ENG`	`@0 cycles @5 13`
C03	`14`	`X`	`FRE`	`@0 Structure 3 dimensions @5 14`
C03	`14`	`X`	`ENG`	`@0 Three dimensional structure @5 14`
C03	`14`	`X`	`SPA`	`@0 Estructura 3 dimensiones @5 14`
C03	`15`	`X`	`FRE`	`@0 Tourbillon @5 15`
C03	`15`	`X`	`ENG`	`@0 Vortex @5 15`
C03	`15`	`X`	`SPA`	`@0 Torbellino @5 15`
C03	`16`	`X`	`FRE`	`@0 Moyenne latitude @5 16`
C03	`16`	`X`	`ENG`	`@0 Mid latitude @5 16`
C03	`16`	`X`	`SPA`	`@0 Latitud media @5 16`
C03	`17`	`2`	`FRE`	`@0 Antarctique @2 NG @5 61`
C03	`17`	`2`	`ENG`	`@0 Antarctica @2 NG @5 61`
C03	`17`	`2`	`SPA`	`@0 Antártico @2 NG @5 61`
C07	`01`	`X`	`FRE`	`@0 Zone polaire @5 17`
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C07	`01`	`X`	`SPA`	`@0 Zona polar @5 17`
C07	`02`	`2`	`FRE`	`@0 Région Polaire @2 564`
C07	`02`	`2`	`ENG`	`@0 polar regions @2 564`
N21				`@1 229`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

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Le document en format XML

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<front><div type="abstract" xml:lang="en">We present Global Ozone Monitoring Experiment-2 (GOME-2) ozone profiles that were operationally retrieved with the KNMI Ozone ProfilE Retrieval Algorithm (OPERA) algorithm for the period September-December 2008. It is shown that it is possible to accurately measure the vertical distribution of stratospheric ozone for Antarctic ozone hole conditions from spectra measured at ultraviolet wavelengths from a nadir viewing instrument. Comparisons with ozone sonde observations from the Neumayer station at the Antarctic coast show a good agreement for various ozone profile shapes representing different phases of the annual recurring ozone hole cycle. A preliminary analysis of the three-dimensional structure of the ozone hole shows for example that at the vortex edges ozone rich mid-latitude middle and upper stratospheric layers can be found over ozone depleted lower stratospheric 'ozone hole' layers. These Antarctic ozone profile observations combined with the daily global coverage of GOME-2 enables the monitoring of the three-dimensional structure of the ozone hole on a daily basis.</div>
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<fC03 i1="04" i2="2" l="ENG"><s0>ozone</s0>
<s5>04</s5>
</fC03>
<fC03 i1="04" i2="2" l="SPA"><s0>Ozono</s0>
<s5>04</s5>
</fC03>
<fC03 i1="05" i2="2" l="FRE"><s0>Surveillance</s0>
<s5>05</s5>
</fC03>
<fC03 i1="05" i2="2" l="ENG"><s0>monitoring</s0>
<s5>05</s5>
</fC03>
<fC03 i1="05" i2="2" l="SPA"><s0>Vigilancia</s0>
<s5>05</s5>
</fC03>
<fC03 i1="06" i2="2" l="FRE"><s0>Etude expérimentale</s0>
<s5>06</s5>
</fC03>
<fC03 i1="06" i2="2" l="ENG"><s0>experimental studies</s0>
<s5>06</s5>
</fC03>
<fC03 i1="07" i2="X" l="FRE"><s0>Algorithme extraction</s0>
<s5>07</s5>
</fC03>
<fC03 i1="07" i2="X" l="ENG"><s0>Retrieval algorithm</s0>
<s5>07</s5>
</fC03>
<fC03 i1="07" i2="X" l="SPA"><s0>Algoritmo extracción</s0>
<s5>07</s5>
</fC03>
<fC03 i1="08" i2="X" l="FRE"><s0>Répartition verticale</s0>
<s5>08</s5>
</fC03>
<fC03 i1="08" i2="X" l="ENG"><s0>Vertical distribution</s0>
<s5>08</s5>
</fC03>
<fC03 i1="08" i2="X" l="SPA"><s0>Distribución vertical</s0>
<s5>08</s5>
</fC03>
<fC03 i1="09" i2="2" l="FRE"><s0>Stratosphère</s0>
<s5>09</s5>
</fC03>
<fC03 i1="09" i2="2" l="ENG"><s0>stratosphere</s0>
<s5>09</s5>
</fC03>
<fC03 i1="09" i2="2" l="SPA"><s0>Estratosfera</s0>
<s5>09</s5>
</fC03>
<fC03 i1="10" i2="2" l="FRE"><s0>Spectre</s0>
<s5>10</s5>
</fC03>
<fC03 i1="10" i2="2" l="ENG"><s0>spectra</s0>
<s5>10</s5>
</fC03>
<fC03 i1="10" i2="2" l="SPA"><s0>Espectro</s0>
<s5>10</s5>
</fC03>
<fC03 i1="11" i2="2" l="FRE"><s0>Longueur onde</s0>
<s5>11</s5>
</fC03>
<fC03 i1="11" i2="2" l="ENG"><s0>wavelength</s0>
<s5>11</s5>
</fC03>
<fC03 i1="12" i2="2" l="FRE"><s0>Instrumentation</s0>
<s5>12</s5>
</fC03>
<fC03 i1="12" i2="2" l="ENG"><s0>instruments</s0>
<s5>12</s5>
</fC03>
<fC03 i1="12" i2="2" l="SPA"><s0>Instrumentación</s0>
<s5>12</s5>
</fC03>
<fC03 i1="13" i2="2" l="FRE"><s0>Cycle</s0>
<s5>13</s5>
</fC03>
<fC03 i1="13" i2="2" l="ENG"><s0>cycles</s0>
<s5>13</s5>
</fC03>
<fC03 i1="14" i2="X" l="FRE"><s0>Structure 3 dimensions</s0>
<s5>14</s5>
</fC03>
<fC03 i1="14" i2="X" l="ENG"><s0>Three dimensional structure</s0>
<s5>14</s5>
</fC03>
<fC03 i1="14" i2="X" l="SPA"><s0>Estructura 3 dimensiones</s0>
<s5>14</s5>
</fC03>
<fC03 i1="15" i2="X" l="FRE"><s0>Tourbillon</s0>
<s5>15</s5>
</fC03>
<fC03 i1="15" i2="X" l="ENG"><s0>Vortex</s0>
<s5>15</s5>
</fC03>
<fC03 i1="15" i2="X" l="SPA"><s0>Torbellino</s0>
<s5>15</s5>
</fC03>
<fC03 i1="16" i2="X" l="FRE"><s0>Moyenne latitude</s0>
<s5>16</s5>
</fC03>
<fC03 i1="16" i2="X" l="ENG"><s0>Mid latitude</s0>
<s5>16</s5>
</fC03>
<fC03 i1="16" i2="X" l="SPA"><s0>Latitud media</s0>
<s5>16</s5>
</fC03>
<fC03 i1="17" i2="2" l="FRE"><s0>Antarctique</s0>
<s2>NG</s2>
<s5>61</s5>
</fC03>
<fC03 i1="17" i2="2" l="ENG"><s0>Antarctica</s0>
<s2>NG</s2>
<s5>61</s5>
</fC03>
<fC03 i1="17" i2="2" l="SPA"><s0>Antártico</s0>
<s2>NG</s2>
<s5>61</s5>
</fC03>
<fC07 i1="01" i2="X" l="FRE"><s0>Zone polaire</s0>
<s5>17</s5>
</fC07>
<fC07 i1="01" i2="X" l="ENG"><s0>Polar region</s0>
<s5>17</s5>
</fC07>
<fC07 i1="01" i2="X" l="SPA"><s0>Zona polar</s0>
<s5>17</s5>
</fC07>
<fC07 i1="02" i2="2" l="FRE"><s0>Région Polaire</s0>
<s2>564</s2>
</fC07>
<fC07 i1="02" i2="2" l="ENG"><s0>polar regions</s0>
<s2>564</s2>
</fC07>
<fN21><s1>229</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
</record>

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   |texte=   Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2
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Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2

Height resolved ozone hole structure as observed by the Global Ozone Monitoring Experiment-2

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