Variation of ionospheric total electron content at crest of equatorial anomaly in China from 1997 to 2004
The periodic variation of TEC data at Xiamen station (geographic coordinate: 24.4°N, 118.1°E; geomagnetic coordinate: 13.2°N, 187.4°E) at crest of equatorial anomaly in China from 1997 to 2004 is analyzed. The characteristic of TEC association with solar activity and geomagnetic activity are also an...
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Veröffentlicht in: | Advances in space research 2012-02, Vol.49 (3), p.539-545 |
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description | The periodic variation of TEC data at Xiamen station (geographic coordinate: 24.4°N, 118.1°E; geomagnetic coordinate: 13.2°N, 187.4°E) at crest of equatorial anomaly in China from 1997 to 2004 is analyzed. The characteristic of TEC association with solar activity and geomagnetic activity are also analyzed. The method of continuous wavelet, cross wavelet and wavelet coherence transform methods have been used. Analysis results show that long-term variations of TEC at Xiamen station are mainly controlled by the variations of solar activities. Several remarkable components including 128–256
days, 256–512
days and 512–1024
days exist in TEC variations. The TEC data at Xiamen station is in anti-phase with geomagnetic Dst index in semiannual time-scale, but this response only exists during high solar activity. Diurnal variation of TEC is studied for different seasons. Some features like the semiannual anomaly and winter anomaly in TEC have been reported. |
doi_str_mv | 10.1016/j.asr.2011.11.008 |
format | Article |
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days, 256–512
days and 512–1024
days exist in TEC variations. The TEC data at Xiamen station is in anti-phase with geomagnetic Dst index in semiannual time-scale, but this response only exists during high solar activity. Diurnal variation of TEC is studied for different seasons. Some features like the semiannual anomaly and winter anomaly in TEC have been reported.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/j.asr.2011.11.008</identifier><identifier>CODEN: ASRSDW</identifier><language>eng</language><publisher>Oxford: Elsevier Ltd</publisher><subject>Astronomy ; Cross wavelet ; Earth, ocean, space ; Equatorial ionization anomaly (EIA) ; Exact sciences and technology ; External geophysics ; Total electron content (TEC) ; Wavelet coherence ; Xiamen station</subject><ispartof>Advances in space research, 2012-02, Vol.49 (3), p.539-545</ispartof><rights>2011 COSPAR</rights><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c359t-77ef4aabcc253abb5bb172c0fd91ea0af6f55f35202559cb012a9f2bac7e688b3</citedby><cites>FETCH-LOGICAL-c359t-77ef4aabcc253abb5bb172c0fd91ea0af6f55f35202559cb012a9f2bac7e688b3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0273117711007678$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,776,780,3536,27903,27904,65309</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=25433529$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Zhenzhong, Xu</creatorcontrib><creatorcontrib>Weimin, Wang</creatorcontrib><creatorcontrib>Ren, Zhang</creatorcontrib><creatorcontrib>Shenggao, Yang</creatorcontrib><title>Variation of ionospheric total electron content at crest of equatorial anomaly in China from 1997 to 2004</title><title>Advances in space research</title><description>The periodic variation of TEC data at Xiamen station (geographic coordinate: 24.4°N, 118.1°E; geomagnetic coordinate: 13.2°N, 187.4°E) at crest of equatorial anomaly in China from 1997 to 2004 is analyzed. The characteristic of TEC association with solar activity and geomagnetic activity are also analyzed. The method of continuous wavelet, cross wavelet and wavelet coherence transform methods have been used. Analysis results show that long-term variations of TEC at Xiamen station are mainly controlled by the variations of solar activities. Several remarkable components including 128–256
days, 256–512
days and 512–1024
days exist in TEC variations. The TEC data at Xiamen station is in anti-phase with geomagnetic Dst index in semiannual time-scale, but this response only exists during high solar activity. Diurnal variation of TEC is studied for different seasons. Some features like the semiannual anomaly and winter anomaly in TEC have been reported.</description><subject>Astronomy</subject><subject>Cross wavelet</subject><subject>Earth, ocean, space</subject><subject>Equatorial ionization anomaly (EIA)</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Total electron content (TEC)</subject><subject>Wavelet coherence</subject><subject>Xiamen station</subject><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWD9-gLdcxNPWJLtpNniS4hcIXtRrmE0nmLJN2iQV-u9NqXgUBuYwz_vOzEvIFWdTzvjsdjmFnKaCcT6txVh_RCa8V7rhuuuPyYQJ1TacK3VKznJeMsaFUmxC_CckD8XHQKOjtcW8_sLkLS2xwEhxRFtSndoYCoZCoVCbMJc9jpstlFj1I4UQVzDuqA90_uUDUJfiinKtVTWigrHugpw4GDNe_vZz8vH48D5_bl7fnl7m96-NbaUujVLoOoDBWiFbGAY5DFwJy9xCcwQGbuakdK0UTEip7VAfAe3EAFbhrO-H9pzcHHzXKW629VKz8tniOELAuM1Gi1YwqWZ9JfmBtCnmnNCZdfIrSDvDmdmnapampmr2qZpaNdWquf51h2xhdAmC9flPKGTX1tt05e4OHNZXvz0mk63HYHHhU03ULKL_Z8sPwYuNKA</recordid><startdate>20120201</startdate><enddate>20120201</enddate><creator>Zhenzhong, Xu</creator><creator>Weimin, Wang</creator><creator>Ren, Zhang</creator><creator>Shenggao, Yang</creator><general>Elsevier Ltd</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20120201</creationdate><title>Variation of ionospheric total electron content at crest of equatorial anomaly in China from 1997 to 2004</title><author>Zhenzhong, Xu ; Weimin, Wang ; Ren, Zhang ; Shenggao, Yang</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c359t-77ef4aabcc253abb5bb172c0fd91ea0af6f55f35202559cb012a9f2bac7e688b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Astronomy</topic><topic>Cross wavelet</topic><topic>Earth, ocean, space</topic><topic>Equatorial ionization anomaly (EIA)</topic><topic>Exact sciences and technology</topic><topic>External geophysics</topic><topic>Total electron content (TEC)</topic><topic>Wavelet coherence</topic><topic>Xiamen station</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zhenzhong, Xu</creatorcontrib><creatorcontrib>Weimin, Wang</creatorcontrib><creatorcontrib>Ren, Zhang</creatorcontrib><creatorcontrib>Shenggao, Yang</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhenzhong, Xu</au><au>Weimin, Wang</au><au>Ren, Zhang</au><au>Shenggao, Yang</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Variation of ionospheric total electron content at crest of equatorial anomaly in China from 1997 to 2004</atitle><jtitle>Advances in space research</jtitle><date>2012-02-01</date><risdate>2012</risdate><volume>49</volume><issue>3</issue><spage>539</spage><epage>545</epage><pages>539-545</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><coden>ASRSDW</coden><abstract>The periodic variation of TEC data at Xiamen station (geographic coordinate: 24.4°N, 118.1°E; geomagnetic coordinate: 13.2°N, 187.4°E) at crest of equatorial anomaly in China from 1997 to 2004 is analyzed. The characteristic of TEC association with solar activity and geomagnetic activity are also analyzed. The method of continuous wavelet, cross wavelet and wavelet coherence transform methods have been used. Analysis results show that long-term variations of TEC at Xiamen station are mainly controlled by the variations of solar activities. Several remarkable components including 128–256
days, 256–512
days and 512–1024
days exist in TEC variations. The TEC data at Xiamen station is in anti-phase with geomagnetic Dst index in semiannual time-scale, but this response only exists during high solar activity. Diurnal variation of TEC is studied for different seasons. Some features like the semiannual anomaly and winter anomaly in TEC have been reported.</abstract><cop>Oxford</cop><pub>Elsevier Ltd</pub><doi>10.1016/j.asr.2011.11.008</doi><tpages>7</tpages></addata></record> |
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subjects | Astronomy Cross wavelet Earth, ocean, space Equatorial ionization anomaly (EIA) Exact sciences and technology External geophysics Total electron content (TEC) Wavelet coherence Xiamen station |
title | Variation of ionospheric total electron content at crest of equatorial anomaly in China from 1997 to 2004 |
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