{"title":"太阳极小期地磁共轭点电离层TEC的变化","authors":"S. Bahari, M. Abdullah, B. Yatim","doi":"10.1109/ICONSPACE.2009.5352647","DOIUrl":null,"url":null,"abstract":"We have studied the variations of TEC at quasi-conjugate points using data obtained from GPS receiver at Syowa station, Antarctica (SYOG) (GC: −69.00° S, 39.58° E; CGM: −66.08°S, 71.65 E°), and Árholt station (ARHO), Iceland (high Arctic region) (GC: 66.19° N, 342.89° E; CGM: 66.37°S, 71.48 E°) for a period in 2007, during the minimum phase of solar cycle 23. The GPS measurements of IGS and IMO network were used to create TEC maps. The time resolution of TEC maps is about 1 hour. The TEC maps show that the maximum TEC value over SYOG is at 1000 UT (1300 LT) while in ARHO is at 1300 UT (UT = LT). March 2007, when it was summer in the southern polar region, the TEC value over SYOG range was higher by 3 TECU than ARHO, which was experiencing winter during that time. This has proved the role of sun in the TEC distribution with photoionization process. The measurements of the TEC variation obtained from GPS during different months at both hemispheres showed symmetry in the median TEC at the conjugate points.","PeriodicalId":360685,"journal":{"name":"2009 International Conference on Space Science and Communication","volume":"44 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2009-12-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Variations of ionospheric TEC at geomagnetic conjugate points during solar minimum\",\"authors\":\"S. Bahari, M. Abdullah, B. Yatim\",\"doi\":\"10.1109/ICONSPACE.2009.5352647\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We have studied the variations of TEC at quasi-conjugate points using data obtained from GPS receiver at Syowa station, Antarctica (SYOG) (GC: −69.00° S, 39.58° E; CGM: −66.08°S, 71.65 E°), and Árholt station (ARHO), Iceland (high Arctic region) (GC: 66.19° N, 342.89° E; CGM: 66.37°S, 71.48 E°) for a period in 2007, during the minimum phase of solar cycle 23. The GPS measurements of IGS and IMO network were used to create TEC maps. The time resolution of TEC maps is about 1 hour. The TEC maps show that the maximum TEC value over SYOG is at 1000 UT (1300 LT) while in ARHO is at 1300 UT (UT = LT). March 2007, when it was summer in the southern polar region, the TEC value over SYOG range was higher by 3 TECU than ARHO, which was experiencing winter during that time. This has proved the role of sun in the TEC distribution with photoionization process. The measurements of the TEC variation obtained from GPS during different months at both hemispheres showed symmetry in the median TEC at the conjugate points.\",\"PeriodicalId\":360685,\"journal\":{\"name\":\"2009 International Conference on Space Science and Communication\",\"volume\":\"44 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2009-12-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2009 International Conference on Space Science and Communication\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/ICONSPACE.2009.5352647\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2009 International Conference on Space Science and Communication","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ICONSPACE.2009.5352647","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
本文利用南极Syowa站(SYOG) GPS接收机(GC: - 69.00°S, 39.58°E;CGM:−66.08°S, 71.65 E°),冰岛(高北极地区)Árholt站(ARHO) (GC: 66.19°N, 342.89°E;CGM: 66.37°S, 71.48 E°),在2007年太阳周期23的最小阶段。利用IGS和IMO网络的GPS测量值制作TEC地图。TEC地图的时间分辨率约为1小时。TEC图显示SYOG的最大TEC值为1000 UT (1300 LT),而ARHO的最大TEC值为1300 UT (UT = LT)。2007年3月,当南极地区处于夏季时,SYOG范围的TEC值比ARHO高3 TECU,此时ARHO正在经历冬季。这证明了太阳在光离过程中TEC分布中的作用。GPS在两个半球不同月份获得的TEC变化测量结果显示,共轭点的TEC中值具有对称性。
Variations of ionospheric TEC at geomagnetic conjugate points during solar minimum
We have studied the variations of TEC at quasi-conjugate points using data obtained from GPS receiver at Syowa station, Antarctica (SYOG) (GC: −69.00° S, 39.58° E; CGM: −66.08°S, 71.65 E°), and Árholt station (ARHO), Iceland (high Arctic region) (GC: 66.19° N, 342.89° E; CGM: 66.37°S, 71.48 E°) for a period in 2007, during the minimum phase of solar cycle 23. The GPS measurements of IGS and IMO network were used to create TEC maps. The time resolution of TEC maps is about 1 hour. The TEC maps show that the maximum TEC value over SYOG is at 1000 UT (1300 LT) while in ARHO is at 1300 UT (UT = LT). March 2007, when it was summer in the southern polar region, the TEC value over SYOG range was higher by 3 TECU than ARHO, which was experiencing winter during that time. This has proved the role of sun in the TEC distribution with photoionization process. The measurements of the TEC variation obtained from GPS during different months at both hemispheres showed symmetry in the median TEC at the conjugate points.