Influence of Quasi-Biennial Oscillation on the Dynamics of Stratospheric Polar Vortices According to Data of Satellite Observations
The lifetime of polar ozone anomalies depends on the phase of quasi-biennial oscillation (QBO). The QBO determines the location of the subtropical critical wind line, which influences the propagation of planetary waves into the stratosphere. As a result, during the westerly phase of the QBO, the str...
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description | The lifetime of polar ozone anomalies depends on the phase of quasi-biennial oscillation (QBO). The QBO determines the location of the subtropical critical wind line, which influences the propagation of planetary waves into the stratosphere. As a result, during the westerly phase of the QBO, the strengthening of a polar vortex is observed, while, during the easterly phase, its weakening is seen, which manifests itself in the dates, duration, and intensity of the stratospheric ozone depletion. Polar ozone anomalies occur inside a strong polar vortex from the end of winter up to spring as a result of the occurrence of heterogeneous and photochemical ozone depletion reactions in the presence of solar radiation. The effect of QBO phases at different isobaric levels on the dynamics of the stratospheric polar vortices are studied on the basis of satellite data from NASA’s Goddard Space Flight Center (GSFC). It is shown that the QBO at the pressure level of 30 hPa has a predominant effect on the dynamics of polar vortices. In the dynamics of the Antarctic polar vortex, it is observed from September to December, especially in October and November; in the dynamics of the Arctic polar vortex, it is pronounced throughout the entire period of its existence. |
doi_str_mv | 10.1134/S0001433823120265 |
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The effect of QBO phases at different isobaric levels on the dynamics of the stratospheric polar vortices are studied on the basis of satellite data from NASA’s Goddard Space Flight Center (GSFC). It is shown that the QBO at the pressure level of 30 hPa has a predominant effect on the dynamics of polar vortices. In the dynamics of the Antarctic polar vortex, it is observed from September to December, especially in October and November; in the dynamics of the Arctic polar vortex, it is pronounced throughout the entire period of its existence.</description><identifier>ISSN: 0001-4338</identifier><identifier>EISSN: 1555-628X</identifier><identifier>DOI: 10.1134/S0001433823120265</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Anomalies ; Antarctic vortex ; Climatology ; Depletion ; Dynamics ; Earth and Environmental Science ; Earth Sciences ; Geophysics/Geodesy ; Ozone ; Ozone anomalies ; Ozone depletion ; Photochemical ozone ; Photochemical reactions ; Photochemicals ; Photochemistry ; Physical Bases and Methods of Studying the Earth from Space ; Planetary waves ; Polar vortex ; Quasi-biennial oscillation ; Satellite data ; Satellite observation ; Satellites ; Solar radiation ; Space flight ; Stratosphere ; Stratospheric polar vortexes ; Stratospheric vortices ; Vortices ; Wave propagation</subject><ispartof>Izvestiya. 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S.</creatorcontrib><title>Influence of Quasi-Biennial Oscillation on the Dynamics of Stratospheric Polar Vortices According to Data of Satellite Observations</title><title>Izvestiya. Atmospheric and oceanic physics</title><addtitle>Izv. Atmos. Ocean. Phys</addtitle><description>The lifetime of polar ozone anomalies depends on the phase of quasi-biennial oscillation (QBO). The QBO determines the location of the subtropical critical wind line, which influences the propagation of planetary waves into the stratosphere. As a result, during the westerly phase of the QBO, the strengthening of a polar vortex is observed, while, during the easterly phase, its weakening is seen, which manifests itself in the dates, duration, and intensity of the stratospheric ozone depletion. Polar ozone anomalies occur inside a strong polar vortex from the end of winter up to spring as a result of the occurrence of heterogeneous and photochemical ozone depletion reactions in the presence of solar radiation. The effect of QBO phases at different isobaric levels on the dynamics of the stratospheric polar vortices are studied on the basis of satellite data from NASA’s Goddard Space Flight Center (GSFC). It is shown that the QBO at the pressure level of 30 hPa has a predominant effect on the dynamics of polar vortices. In the dynamics of the Antarctic polar vortex, it is observed from September to December, especially in October and November; in the dynamics of the Arctic polar vortex, it is pronounced throughout the entire period of its existence.</description><subject>Anomalies</subject><subject>Antarctic vortex</subject><subject>Climatology</subject><subject>Depletion</subject><subject>Dynamics</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Geophysics/Geodesy</subject><subject>Ozone</subject><subject>Ozone anomalies</subject><subject>Ozone depletion</subject><subject>Photochemical ozone</subject><subject>Photochemical reactions</subject><subject>Photochemicals</subject><subject>Photochemistry</subject><subject>Physical Bases and Methods of Studying the Earth from Space</subject><subject>Planetary waves</subject><subject>Polar vortex</subject><subject>Quasi-biennial oscillation</subject><subject>Satellite data</subject><subject>Satellite observation</subject><subject>Satellites</subject><subject>Solar radiation</subject><subject>Space flight</subject><subject>Stratosphere</subject><subject>Stratospheric polar vortexes</subject><subject>Stratospheric vortices</subject><subject>Vortices</subject><subject>Wave propagation</subject><issn>0001-4338</issn><issn>1555-628X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp1kEtLAzEUhYMoWKs_wF3A9WgenTRd1tZHoVClKu6GJHOnTZkmNckIXfvHnbaCCxEunMU537lwELqk5JpS3ruZE0Joj3PJOGWEifwIdWie55lg8v0YdXZ2tvNP0VmMK0IE65F-B31NXFU34AxgX-HnRkWb3Vpwzqoaz6Kxda2S9Q63l5aAx1un1tbEXXqegko-bpYQrMFPvlYBv_mQrIGIh8b4UFq3wMnjsUpqT6gEdW0T4JmOED731fEcnVSqjnDxo130en_3MnrMprOHyWg4zQwTMmWaUa25NsQIzYCCrhRXZU61yQdalKWsWNkvwVQaSG6IJkZTMFJxIShXMudddHXo3QT_0UBMxco3wbUvCzZgUsqBaLfsInpImeBjDFAVm2DXKmwLSord1sWfrVuGHZjYZt0Cwm_z_9A3X5eDpw</recordid><startdate>20231201</startdate><enddate>20231201</enddate><creator>Zuev, V. V.</creator><creator>Maslennikova, E. A.</creator><creator>Savelieva, E. S.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>20231201</creationdate><title>Influence of Quasi-Biennial Oscillation on the Dynamics of Stratospheric Polar Vortices According to Data of Satellite Observations</title><author>Zuev, V. V. ; Maslennikova, E. A. ; Savelieva, E. S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c268t-b21bb3bc0c6b2e1ebfa3ad51bc59b6dd8f2d7decfbe05c0b0cb1ec8a36613a853</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Anomalies</topic><topic>Antarctic vortex</topic><topic>Climatology</topic><topic>Depletion</topic><topic>Dynamics</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Geophysics/Geodesy</topic><topic>Ozone</topic><topic>Ozone anomalies</topic><topic>Ozone depletion</topic><topic>Photochemical ozone</topic><topic>Photochemical reactions</topic><topic>Photochemicals</topic><topic>Photochemistry</topic><topic>Physical Bases and Methods of Studying the Earth from Space</topic><topic>Planetary waves</topic><topic>Polar vortex</topic><topic>Quasi-biennial oscillation</topic><topic>Satellite data</topic><topic>Satellite observation</topic><topic>Satellites</topic><topic>Solar radiation</topic><topic>Space flight</topic><topic>Stratosphere</topic><topic>Stratospheric polar vortexes</topic><topic>Stratospheric vortices</topic><topic>Vortices</topic><topic>Wave propagation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zuev, V. V.</creatorcontrib><creatorcontrib>Maslennikova, E. A.</creatorcontrib><creatorcontrib>Savelieva, E. S.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Izvestiya. Atmospheric and oceanic physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zuev, V. V.</au><au>Maslennikova, E. A.</au><au>Savelieva, E. S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Influence of Quasi-Biennial Oscillation on the Dynamics of Stratospheric Polar Vortices According to Data of Satellite Observations</atitle><jtitle>Izvestiya. Atmospheric and oceanic physics</jtitle><stitle>Izv. Atmos. Ocean. Phys</stitle><date>2023-12-01</date><risdate>2023</risdate><volume>59</volume><issue>10</issue><spage>1307</spage><epage>1313</epage><pages>1307-1313</pages><issn>0001-4338</issn><eissn>1555-628X</eissn><abstract>The lifetime of polar ozone anomalies depends on the phase of quasi-biennial oscillation (QBO). The QBO determines the location of the subtropical critical wind line, which influences the propagation of planetary waves into the stratosphere. As a result, during the westerly phase of the QBO, the strengthening of a polar vortex is observed, while, during the easterly phase, its weakening is seen, which manifests itself in the dates, duration, and intensity of the stratospheric ozone depletion. Polar ozone anomalies occur inside a strong polar vortex from the end of winter up to spring as a result of the occurrence of heterogeneous and photochemical ozone depletion reactions in the presence of solar radiation. The effect of QBO phases at different isobaric levels on the dynamics of the stratospheric polar vortices are studied on the basis of satellite data from NASA’s Goddard Space Flight Center (GSFC). It is shown that the QBO at the pressure level of 30 hPa has a predominant effect on the dynamics of polar vortices. In the dynamics of the Antarctic polar vortex, it is observed from September to December, especially in October and November; in the dynamics of the Arctic polar vortex, it is pronounced throughout the entire period of its existence.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0001433823120265</doi><tpages>7</tpages></addata></record> |
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subjects | Anomalies Antarctic vortex Climatology Depletion Dynamics Earth and Environmental Science Earth Sciences Geophysics/Geodesy Ozone Ozone anomalies Ozone depletion Photochemical ozone Photochemical reactions Photochemicals Photochemistry Physical Bases and Methods of Studying the Earth from Space Planetary waves Polar vortex Quasi-biennial oscillation Satellite data Satellite observation Satellites Solar radiation Space flight Stratosphere Stratospheric polar vortexes Stratospheric vortices Vortices Wave propagation |
title | Influence of Quasi-Biennial Oscillation on the Dynamics of Stratospheric Polar Vortices According to Data of Satellite Observations |
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