Optical-electronic Theodolite Calibration with Star in Range

张薇 Zhang Wei, 柳玉晗 Liu Yu-han, 李世诚 Li Shi-cheng
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引用次数: 1

Abstract

Optical-electronic theodolite is a primary measuring equipment of external trajectory.It's precision must be regularly calibrated in the course of use in order to meet the requirements of measuring tasks.The methods of optical-eletronic theodolite calibration in the range were studied.The course of measuring star was introduced,and the criterion of selecting star and the arithmetic of computing star theory were explained.The mathematic model was established after obtaining the measurement value of the star and the errors of the theodolite were calculated by using the least square method.At last,several factors of the calibration method with star were set forth.The computing results were checked by using factual devices.The result in range accorded with that of inner detection.It was showed that the calibration method with star in range was right.
星距内光电经纬仪标定
光电经纬仪是外弹道的主要测量设备。为了满足测量任务的要求,在使用过程中必须对其精度进行定期校准。研究了该范围内光电经纬仪的标定方法。介绍了测量恒星的过程,说明了选择恒星的准则和计算恒星理论的算法。在获得该星的测量值后,建立数学模型,利用最小二乘法计算经纬仪的误差。最后,阐述了星形定标方法的几个影响因素。用实际装置对计算结果进行了验证。测距结果与内测结果一致。结果表明,星距标定方法是正确的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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