Analysis of the ionosphere wave-motion with GPS  

作　　者：ZHANGHongping ZHUWenyao PENGJunhuan HUANGCheng 

机构地区：[1]ShanghaiAstronomicalObservatory,ChineseAcademyofSciences,Shanghai200030,China//GraduateSchooloftheChineseAcademyofSciences,Beijing100039,China [2]ShanghaiAstronomicalObservatory,ChineseAcademyofSciences,Shanghai200030,China//KeyLaboratoryofAdvancedEngineeringSurveyofSBSM,TongjiUniversity,Shanghai200092,China [3]ShanghaiAstronomicalObservatory,ChineseAcademyofSciences,Shanghai200030,China

出　　处：《Chinese Science Bulletin》2005年第13期1373-1381,共9页

基　　金：supported by the 100-Talent Fund of the Chinese Academy of Sciences in Astro-geodynamic Center of Shanghai Astronomical Observatory;the National Natural Science Foundation of China(Grant No.40174009);the Knowledge Creative Project of the Chinese Academy of Sciences(Grant No.KJCX2-SW-T1);the Shanghai Scientific Technology Development Fund(Grant No.JC14012);the Guangxi Fund for Youth(Grant No.9912008).

摘　　要：Precise vertical total electron contents (VTEC) and its time variation have been obtained by using GPS dual-frequency observations collected by the continuously operating GPS tracking stations distributed over China. Us-ing VTEC data, the wave-motion appearing in the iono-sphere on November 3, 2003 is monitored and analyzed when a small solar flare happened. Detailed discussion with the VTEC and its change rate series, which are derived from the observations (data) from PRN23 satellite, indicates that the wave-motion mainly contains two dominant frequencies and propagates almost along the meridian line toward south. Additionally, the fluctuation of the mean VTEC has been calculated in a regional Single Layer Model (SLM) iono-spheric shell in the range of N28.0°―34.0° and E118.0°―123.0°. The spectral analysis and the multi-resolution analy-sis of mean VTEC time series show that the periods of these two components of the wave-motion at middle altitude are around 60 and 25 min separately, and the amplitudes can be up to 1.0―2.0 TECU and 0.4―0.7 TECU respectively. Mean- while, the relative motion between the wave-motion and the Ionosphere Pierce Points (IPPs), which are defined as the cross points between the line-of-sight of the GPS signals and the SLM thin shell, reveals that the traveling speeds of the two components are about 120―150 m/s and 30―40 m/s respectively.Precise vertical total electron contents (VTEC) and its time variation have been obtained by using GPS dual-frequency observations collected by the continuously operating GPS tracking stations distributed over China. Using VTEC data, the wave-motion appearing in the ionosphere on November 3, 2003 is monitored and analyzed when a small solar flare happened. Detailed discussion with the VTEC and its change rate series, which are derived from the observations (data) from PRN23 satellite, indicates that the wave-motion mainly contains two dominant frequencies and propagates almost along the meridian line toward south. Additionally, the fluctuation of the mean VTEC has been calculated in a regional Single Layer Model (SLM) ionospheric shell in the range of N28.0 degrees-34.0 degrees and E118.0 degrees-123.0 degrees. The spectral analysis and the multi-resolution analysis of mean VTEC time series show that the periods of these two components of the wave-motion at middle altitude are around 60 and 25 min separately, and the amplitudes can be up to 1.0 - 2.0 TECU and 0.4 - 0.7 TECU respectively. Meanwhile, the relative motion between the wave-motion and the Ionosphere Pierce Points (IPPs), which are defined as the cross points between the line-of-sight of the GPS signals and the SLM thin shell, reveals that the traveling speeds of the two components are about 120-150 m/s and 30-40 m/s respectively.

关 键 词：电离波 GPS 全球定位系统 光谱分析 微波分析 

分 类 号：O433.4[机械工程—光学工程] P228.4[理学—光学]