望远镜的基墩设计方案是大型望远镜设计方案的重要组成部分，也是决定望远镜能否进行稳定和高精度观测的重要先决条件。由于Dome A地区温度极低，冰层厚度达到3000m，一般的望远镜基墩处理方法无法应用，需要进行特别的设计和处理。本项目主要针对Dome A地区的望远镜的基墩的参数化设计方法进行了研究，其研究的内容主要包括1）Dome A地区冰面的0-10米深度范围的雪冰强度分析；2）获取检测Dome A地区冰面的地基承载力方法的研究；3）Dome A天文望远镜的基墩结构的参数化设计及分析方法的研究。本项目希望通过研究一种望远镜的基墩进行参数化设计的技术，使得未来通过输入相应的望远镜及塔架圆顶的总载重量就可以分析出基墩的大小、结构形式，进而分析出需要的天文场地的面积及地基挖掘深度等条件，减少今后Dome A地区大望远镜的基墩建造的设计时间及现场施工时间。

The foundation design of the telescope is the important part in the design of the telescope, and also the prerequisite of the stability and high accuracy of the telescope. Because of the low temperature and the 3000m ice thickness, the normal treatment of the telescope foundation can not be used in Dome A. The special design of the foundation for the large telescope is urgently needed. The project is mainly focus on research of the Parametric Design method of the Telescope Foundation in Dome A. And the study is mainly included in 3 Parts:1) the ice strength analysis in 10m deep from the surface 2)the method of testing the ice load capacity in Dome A 3)the parametric design method of the telescope foundation in Dome A. If the project successes, the size, structure of the foundation can be quickly got after entering the total load of the telescope ,the tower , and the dome. It can also get the size of the Astronomical facility field and the excavation depth of the foundation in order to reduce the foundation design time and the construction time in Dome A