風云四號靜止氣象衛星測距站坐標測量點的確定及修正
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風云四號02批氣象衛星工程地面應用系統項目資助


Correction and Confirmation of Coordinate Measurement Points for FY-4 Ranging Stations
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    摘要:

    風云四號(FY4)靜止氣象衛星是通過測量多個地面站到衛星的距離實現對衛星的軌道確定和預報,所以測距站站址坐標是影響定軌精度的主要因素之一。星地間距離通常是指地面天線相位中心到衛星天線相位中心之間的距離,但是FY4測距站天線的相位中心無法用作測距距離起始參考點和站址坐標測量點。本文針對FY4測距站簡易半轉臺天線的特殊結構,結合卡塞格倫天線的工作原理,確定出測距距離起始參考點及站址坐標測量點,并給出這兩者之間距離的修正算法。最后根據FY4衛星太空分布位置及各個測距站跟蹤狀況分析了修正結果,并對在工程中實施方法提出了建議。

    Abstract:

    The FY4 geostationary meteorological satellite gets its orbit determination and prediction through ranging the distances from different ground stations to the satellite, so the coordinates of each station site are one of main factors which influence the accuracy of the orbit determination. The satelliteground distance is the distance from the antenna phase center of a ground station to that of the satellite in general, but the antenna phase center of the FY4 ranging station antenna cannot be used to determine the starting reference point of the ranging distance and site coordinate measuring point. On the basis of the theory of the Cassegrain antenna, the following are discussed: where the starting point of ranging is and how to fix the point of coordinates to measure in the condition of the special structure of the antenna. The correction algorithm is given from coordinate measurement point to the ranging start point. Taking the FY4B antenna for an example, the result of correction is analyzed according to the actual condition that five ground stations follow the satellites distributed in seven different sites of space. Finally, suggestions are provided for practical application.

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賈耀紅,裘奕,郭強.風云四號靜止氣象衛星測距站坐標測量點的確定及修正[J].氣象科技,2021,49(3):342~347

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  • 收稿日期:2020-07-24
  • 定稿日期:2020-10-23
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  • 在線發布日期: 2021-06-23
  • 出版日期: 2021-06-30
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