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A method to improve the accuracy of low orbit satellite predietion

机译:一种提高低轨道卫星预测精度的方法

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In this method, the orbit elements a, i, OMEGA , zeta chemical c sin omega , eta chemical bounds c cos omega and lambda M+ omega derived from IRV data are taken as basic variables in numcrical integration. By these elements the polynomial's degree of the interpolation can be decreased. The cheange of x-coordinate axis to Mean Equinox decreases the innfluence of the error of the proedicted TI-UTC. The usage of up date SLR data ean improve the orbit elements of satellites. The order and degrce of the Earth's spherical harmonic perturbation are extended to 20 x 20. The solar and lunar coordinates are improved to about 2', that can further improve the solar and hunar perturbations. The light proessure perturbation, the air drag perturbation, and the influcnecs from the coordinate system and the polar motion transformation are also taken into account. The improved satellite prediction proeedure would be available to the laser satellite observation at the daylight.
机译:在该方法中,轨道元素A,I,Omega,Zeta Compy C Sup Omega,ETA化学界C COS Omega和λM+ Omega源自IRV数据的基本变量在数值积分中被视为基本变量。通过这些元素,可以减少多项式的内插度。 X坐标轴的Cheange均衡Equinox会降低所获用的Ti-UTC的误差的innfluence。使用UP日期SLR数据EAN改善卫星的轨道元素。地球球形谐波扰动的顺序和探测延伸至20×20.太阳能和月球坐标改善到大约2',可以进一步改善太阳能和堤坝的扰动。还考虑了光线扰动,空气阻力扰动和来自坐标系和极性运动变换的粉扑再现。改进的卫星预测装置将在白天的激光卫星观察中使用。

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