摘要
选择最好的天文台址放置大口径望远镜一直是天文学家追求的目标.我国在南极的天文项目近几年得到了快速发展,对南极区域的光学湍流时空分布进行测量和分析,是一项亟待开展的基础性天文工作.本文主要介绍研制的移动式大气参数测量系统,用于南极天文选址,得到了在泰山站近地面常规气象参数和大气湍流的初步测量结果.
Astronomers have always sought the best locations for their large aperture telescopes.Chinese Antarctic astronomy began to flourish in recent years,for the measurement and analysis of optical turbulence temporal and spatial distribution in Antarctic region,as well as beginning a site testing programme to assess the quality of the plateau for astronomy,is an urgent need to carry out the basic astronomical work.This paper introduces a mobile atmospheric parameter measuring system for Antarctic astronomy site testing,and preliminary measurement results of atmospheric turbulence in surface layer at Antarctic Taishan Station.
出处
《安徽师范大学学报（自然科学版）》
CAS
北大核心
2014年第6期511-514,共4页
Journal of Anhui Normal University(Natural Science)
基金
国家自然科学基金项目(41275020)资助
关键词
天文选址
光学湍流
移动式测量系统
astronomical site testing
optical turbulence
mobile measuring system
