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????IGS?????????????TEC?仯???????
引用本文:时爽爽,黄劲松,冯建迪,谭先科.????IGS?????????????TEC?仯???????[J].大地测量与地球动力学,2015,35(2):293-297.
作者姓名:时爽爽  黄劲松  冯建迪  谭先科
作者单位:武汉大学测绘学院,武汉市珞喻路129号, 430079
摘    要:????1999~2009???IGS????????????????(TEC)????????????TEC???????I????dc????????????I????nc?????????仯??????仯????????о????????????????????????????????I????dc???????????????????????????????????????????????????????????????????????????I????dc?????????仯??????????????I????nc????????γ????????а???仯??????????I????dc???????I????nc????????仯????????????仯???仯????????????????85%?????????I????dc????????????????????????I????dc???????I????nc?????????仯?????澭γ??仯???????????????????仯??????????????????????I????dc????????I????nc?????????????P????????????????????????????0.9???????????D????st????K??p??A??p???????????????????????????С??0.4??????????????????????????????????????????TEC????仯????????????á?

关 键 词:IGS  TEC  ????仯  ??????  ????????  
收稿时间:2014-03-20

Analysis of TEC Variation Characteristics in Daytime and Nighttime Based on the IGS Data
SHI Shuangshuang,HUANG Jinsong,FENG Jiandi,TAN Xianke.Analysis of TEC Variation Characteristics in Daytime and Nighttime Based on the IGS Data[J].Journal of Geodesy and Geodynamics,2015,35(2):293-297.
Authors:SHI Shuangshuang  HUANG Jinsong  FENG Jiandi  TAN Xianke
Institution:School of Geodesy and Geomatics, Wuhan University, 129 Luoyu Road, Wuhan 430079, China
Abstract:Based on 1999~2009 total electron content (TEC) data from IGS, we studied semiannual and seasonal variations of the global TEC in the daytime (Idc) and nighttime (Inc) as well as solar and geomagnetic effects on these variations. The main features are outlined as follows: the maximum values of Idc commonly appear in equinox seasons| in the northern ‘near-pole’ region and south America, the semiannual variation character of Idc is significant. Inc has only semiannual variation at low latitudes, and the semiannual variation of Idc and Inc change with the solar activity. At high solar activity years, in more than 85% area of the globe, the maximum value of Idc appears in equinox seasons.  Seasonal variation of Idc and Inc change with latitude and longitude, and seasonal variation is apparent at high solar activity years. The variation of Idc and Inc correlates well with the solar P index, where the correlation coefficient reached 0.9. However, it poorly correlated with geomagnetic Dst, Kp, Ap index, where the correlation coefficient is less than 0.4. We further demonstrate that ionosphere photochemical production rate, which is controlled by solar zenith angle, plays a major role in the overall variation of TEC.
Keywords:IGS  TEC  semiannual variation  seasonal variation  correlation analysis
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