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Spin motion of the AJISAI satellite derived from spectral analysis of laser ranging data

机译:通过对激光测距数据进行频谱分析得出的AJISAI卫星的自旋运动

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The spin rate of the geodetic satellite AJISAI was derived through a spectral analysis of laser range data obtained by precise high-return-rate tracking stations. This new analysis method utilizes the directional dependence of the target optical depth resulting from the sparse distribution of corner cube reflectors on the satellite surface. The third and sixth harmonics of the spin rate were found to be dominant in the pass-by-pass spectral analysis of the full-rate range residuals from multiphoton laser ranging systems. Accumulating hundreds of passes, the analysis results gave the slowdown of AJISAI's spinning from 1997 to 1998. Its trend was almost identical to the conventional flash observation. Although the spin rate derived from this method was not as precise as the conventional one, it can provide global spatial coverage and continuous time coverage to monitor the spin motion. This is a new approach to research satellite orientation and orbit and is applicable to other satellites.
机译:大地卫星AJISAI的自旋速率是通过对精确的高返回率跟踪站获得的激光测距数据进行光谱分析得出的。这种新的分析方法利用了目标光学深度的方向依赖性,这是由于卫星表面上的角锥反射镜稀疏分布所致。发现自旋速率的三次谐波和三次谐波在多光子激光测距系统的全速率范围残差的旁路光谱分析中占主导地位。通过累积数百次通过,分析结果使AJISAI的旋转速度从1997年到1998年有所放缓。其趋势几乎与常规的闪光观测相同。尽管从此方法得出的旋转速率不如传统方法精确,但它可以提供全局空间覆盖范围和连续时间覆盖范围以监视旋转运动。这是研究卫星定向和轨道的一种新方法,适用于其他卫星。

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