摘要
本文给出了处理天王星卫星CCD图象位置资料的新方法 ,并将我们在 1 995年取得的观测资料与两种理论模型位置进行了比较计算 。
In this paper, we provid some new methods of reduction for positioning measurements of Uranian satellites on CCD images. The observations we got in 1995 are compared with the calculated positions from the two theories. The analysis of the CCD observations for the five major Uranian satellites has shown that positioning precision has been improved greatly.
基金
国家自然科学基金委员会支持项目
中国科学院天文委员会基金支持项目
