Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW
The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index,...
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Veröffentlicht in: | Science China. Earth sciences 2017-04, Vol.60 (4), p.776-785 |
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creator | Mo, XiaoHua Zhang, DongHe Goncharenko, Larisa Zhang, ShunRong Hao, YongQiang Xiao, Zuo Pei, JiaZheng Yoshikawa, Akimasa Chau, HaDuyen |
description | The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index, and solar flux index during the 2002–2003 sudden stratospheric warming (SSW) event. Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics. |
doi_str_mv | 10.1007/s11430-016-0096-y |
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Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics.</description><identifier>ISSN: 1674-7313</identifier><identifier>EISSN: 1869-1897</identifier><identifier>DOI: 10.1007/s11430-016-0096-y</identifier><language>eng</language><publisher>Beijing: Science China Press</publisher><subject>Climate change ; Earth and Environmental Science ; Earth Sciences ; Equator ; Geophysics ; Ionization ; Latitude ; Magnetic fields ; Meteorology ; Research Paper ; Stratosphere</subject><ispartof>Science China. Earth sciences, 2017-04, Vol.60 (4), p.776-785</ispartof><rights>Science China Press and Springer-Verlag Berlin Heidelberg 2017</rights><rights>Science China Earth Sciences is a copyright of Springer, 2017.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c349t-1282ae08b83388ee55ee78fe48cb36643a35b59a142c2acce33bd423745797d63</citedby><cites>FETCH-LOGICAL-c349t-1282ae08b83388ee55ee78fe48cb36643a35b59a142c2acce33bd423745797d63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11430-016-0096-y$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11430-016-0096-y$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27922,27923,41486,42555,51317</link.rule.ids></links><search><creatorcontrib>Mo, XiaoHua</creatorcontrib><creatorcontrib>Zhang, DongHe</creatorcontrib><creatorcontrib>Goncharenko, Larisa</creatorcontrib><creatorcontrib>Zhang, ShunRong</creatorcontrib><creatorcontrib>Hao, YongQiang</creatorcontrib><creatorcontrib>Xiao, Zuo</creatorcontrib><creatorcontrib>Pei, JiaZheng</creatorcontrib><creatorcontrib>Yoshikawa, Akimasa</creatorcontrib><creatorcontrib>Chau, HaDuyen</creatorcontrib><title>Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW</title><title>Science China. Earth sciences</title><addtitle>Sci. China Earth Sci</addtitle><description>The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index, and solar flux index during the 2002–2003 sudden stratospheric warming (SSW) event. Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics.</description><subject>Climate change</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Equator</subject><subject>Geophysics</subject><subject>Ionization</subject><subject>Latitude</subject><subject>Magnetic fields</subject><subject>Meteorology</subject><subject>Research Paper</subject><subject>Stratosphere</subject><issn>1674-7313</issn><issn>1869-1897</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kcFq3DAURU1oIGGSD-hO0E03aiQ925KXYUjTwoQsJqFLoZHfJBpsaUayA5NV-w39w3xJZNxFKVSbK6FzH497i-IjZ184Y_IqcV4Co4zXlLGmpseT4pyruqFcNfJDvteypBI4nBWXKe1YPpB_hDwvft1hdK0L3nSkDy_Yox9I2BIf4vCM0RPjW5LCOD_wMJohRJfhbHGvZsiSkdCb7khsxDQk4jzJNLkxaaDXyRlPEtrsIu0YnX8igjHx9vN3FiDr9Y-L4nRruoSXf3RRPH69eVh-o6v72-_L6xW1UDYD5UIJg0xtFIBSiFWFKNUWS2U3UNclGKg2VWN4Kaww1iLApi0FyLKSjWxrWBSf57n7GA5j3lT3LlnsOuMxjEnnrLiSAGJCP_2D7sIYc0QTpaBiFa95pvhM2RhSirjV--h6E4-aMz31oudedO5FT73oY_aI2ZP2UxYY_5r8X9M7ccqREw</recordid><startdate>20170401</startdate><enddate>20170401</enddate><creator>Mo, XiaoHua</creator><creator>Zhang, DongHe</creator><creator>Goncharenko, Larisa</creator><creator>Zhang, ShunRong</creator><creator>Hao, YongQiang</creator><creator>Xiao, Zuo</creator><creator>Pei, JiaZheng</creator><creator>Yoshikawa, Akimasa</creator><creator>Chau, HaDuyen</creator><general>Science China Press</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>M2P</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>20170401</creationdate><title>Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW</title><author>Mo, XiaoHua ; Zhang, DongHe ; Goncharenko, Larisa ; Zhang, ShunRong ; Hao, YongQiang ; Xiao, Zuo ; Pei, JiaZheng ; Yoshikawa, Akimasa ; Chau, HaDuyen</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c349t-1282ae08b83388ee55ee78fe48cb36643a35b59a142c2acce33bd423745797d63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Climate change</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Equator</topic><topic>Geophysics</topic><topic>Ionization</topic><topic>Latitude</topic><topic>Magnetic fields</topic><topic>Meteorology</topic><topic>Research Paper</topic><topic>Stratosphere</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mo, XiaoHua</creatorcontrib><creatorcontrib>Zhang, DongHe</creatorcontrib><creatorcontrib>Goncharenko, Larisa</creatorcontrib><creatorcontrib>Zhang, ShunRong</creatorcontrib><creatorcontrib>Hao, YongQiang</creatorcontrib><creatorcontrib>Xiao, Zuo</creatorcontrib><creatorcontrib>Pei, JiaZheng</creatorcontrib><creatorcontrib>Yoshikawa, Akimasa</creatorcontrib><creatorcontrib>Chau, HaDuyen</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Water Resources Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>ProQuest Central Student</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Science China. Earth sciences</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mo, XiaoHua</au><au>Zhang, DongHe</au><au>Goncharenko, Larisa</au><au>Zhang, ShunRong</au><au>Hao, YongQiang</au><au>Xiao, Zuo</au><au>Pei, JiaZheng</au><au>Yoshikawa, Akimasa</au><au>Chau, HaDuyen</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW</atitle><jtitle>Science China. Earth sciences</jtitle><stitle>Sci. China Earth Sci</stitle><date>2017-04-01</date><risdate>2017</risdate><volume>60</volume><issue>4</issue><spage>776</spage><epage>785</epage><pages>776-785</pages><issn>1674-7313</issn><eissn>1869-1897</eissn><abstract>The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index, and solar flux index during the 2002–2003 sudden stratospheric warming (SSW) event. Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics.</abstract><cop>Beijing</cop><pub>Science China Press</pub><doi>10.1007/s11430-016-0096-y</doi><tpages>10</tpages></addata></record> |
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subjects | Climate change Earth and Environmental Science Earth Sciences Equator Geophysics Ionization Latitude Magnetic fields Meteorology Research Paper Stratosphere |
title | Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW |
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