地球物理学报
地毬物理學報
지구물이학보
2010年
1期
22-29
,共8页
温晋%万卫星%丁锋%乐新安%佘承莉%刘立波
溫晉%萬衛星%丁鋒%樂新安%佘承莉%劉立波
온진%만위성%정봉%악신안%사승리%류립파
TEC%映射函数%等离子体层%电离层质心高度
TEC%映射函數%等離子體層%電離層質心高度
TEC%영사함수%등리자체층%전리층질심고도
Total Electronic Content%Mapping function%Plasmasphere%Ionospheric centroid
利用GPS信标测量获得的电离层电子浓度总含量(TEC)是沿电波路径的斜向TEC.理论研究和实际应用中,常常需要通过映射函数将斜向TEC转换为垂直方向的TEC,这在当前主要采用对电子浓度分布模型的数值积分得到模型映射函数来实现.本文在考察现有不同模型映射函数的基础上,又提出了一种源于实际观测的实验映射函数的概念与估算方法.我们利用IGS的全球GPS观测站的斜向TEC和JPL提供的垂直TEC数据获得了2006年期间的实验映射函数,并对所得结果进行了初步统计分析.在卫星天顶角较小时,上述实验映射函数和模型映射函数之间相差甚微,均可很好描述垂直TEC与斜TEC之间关系;但卫星天顶角较大时,实验映射函数和常用的模型映射函数之间存在明显差异.本文认为,这种差异主要是因为现有模型映射函数中没有考虑到等离子体层的贡献.我们认为采用基于实验映射函数的模式,或者通过考虑等离子体层的贡献对现有模型映射函数进行改进,可以有效提高电离层TEC的估算精度.
利用GPS信標測量穫得的電離層電子濃度總含量(TEC)是沿電波路徑的斜嚮TEC.理論研究和實際應用中,常常需要通過映射函數將斜嚮TEC轉換為垂直方嚮的TEC,這在噹前主要採用對電子濃度分佈模型的數值積分得到模型映射函數來實現.本文在攷察現有不同模型映射函數的基礎上,又提齣瞭一種源于實際觀測的實驗映射函數的概唸與估算方法.我們利用IGS的全毬GPS觀測站的斜嚮TEC和JPL提供的垂直TEC數據穫得瞭2006年期間的實驗映射函數,併對所得結果進行瞭初步統計分析.在衛星天頂角較小時,上述實驗映射函數和模型映射函數之間相差甚微,均可很好描述垂直TEC與斜TEC之間關繫;但衛星天頂角較大時,實驗映射函數和常用的模型映射函數之間存在明顯差異.本文認為,這種差異主要是因為現有模型映射函數中沒有攷慮到等離子體層的貢獻.我們認為採用基于實驗映射函數的模式,或者通過攷慮等離子體層的貢獻對現有模型映射函數進行改進,可以有效提高電離層TEC的估算精度.
이용GPS신표측량획득적전리층전자농도총함량(TEC)시연전파로경적사향TEC.이론연구화실제응용중,상상수요통과영사함수장사향TEC전환위수직방향적TEC,저재당전주요채용대전자농도분포모형적수치적분득도모형영사함수래실현.본문재고찰현유불동모형영사함수적기출상,우제출료일충원우실제관측적실험영사함수적개념여고산방법.아문이용IGS적전구GPS관측참적사향TEC화JPL제공적수직TEC수거획득료2006년기간적실험영사함수,병대소득결과진행료초보통계분석.재위성천정각교소시,상술실험영사함수화모형영사함수지간상차심미,균가흔호묘술수직TEC여사TEC지간관계;단위성천정각교대시,실험영사함수화상용적모형영사함수지간존재명현차이.본문인위,저충차이주요시인위현유모형영사함수중몰유고필도등리자체층적공헌.아문인위채용기우실험영사함수적모식,혹자통과고필등리자체층적공헌대현유모형영사함수진행개진,가이유효제고전리층TEC적고산정도.
The TEC data obtained from GPS is actually the slant TEC, i.e., the integration of electronic density along the GPS signal path. In many applications the slant TEC should be converted into vertical TEC. This is done by the so called mapping function which is usually determined by certain models of electron density profile. In this paper we proposed a new method to obtain mapping functions from TEC observation of GPS network. We first discuss the Single Layer Model (SLM), or the peak electron density height for the Chapman Model, and found that the value of the mapping function decreases obviously with the increase of the ionospheric height. We then estimated the'experimental mapping function' from the observation of vertical TEC (from JPL GIMs) and slant TEC (from IGS GPS data) during the whole year of 2006. After the comparison between both results, we find the values of the mapping functions from experimental data are much larger than that from the model with reasonable ionospheric height (e.g., 400 km SLM height), when the zenith angle is large enough. We attribute this to the effect of the plasmasphere which exists above about 1000 km altitude hence may increase the effective 'ionospheric height'. It is concluded that the present experimental results may be used to model or improve the vertical TEC mapping function. This might be helpful for retrieving TEC from GPS network.