摘要
本文介绍了对中星仪星象光子数据进行预处理的方法和程序,对星象定位进行归(?)方法和程序,最后给出了定位结果和精度。其平均内符合精度小于3mS。
This paper introduces the main noise sources in the observation are analysed and the data procession and reduction are described. As an example, the results of the reduction are given, showing that the inner average precision is less than 3ms.
