中国光学
中國光學
중국광학
CHINESE JOURNAL OF OPTICS
2012年
1期
12-19
,共8页
曹召良%李小平%宣丽%穆全全%胡立发%彭增辉%刘永刚%姚丽双
曹召良%李小平%宣麗%穆全全%鬍立髮%彭增輝%劉永剛%姚麗雙
조소량%리소평%선려%목전전%호립발%팽증휘%류영강%요려쌍
自适应光学%液晶波前校正器%校正频率%大气湍流
自適應光學%液晶波前校正器%校正頻率%大氣湍流
자괄응광학%액정파전교정기%교정빈솔%대기단류
adaptive optics%liquid crystal wavefront corrector%correction frequency%atmospheric turbulence
概述了中科院长春光学精密机械与物理研究所(长春光机所)在液晶自适应光学方面的研究进展。针对液晶自适应光学技术存在的能量利用率低和校正频率慢的两大国际难题,液晶自适应光学研究组采取了一系列有效措施,不但攻克了能量利用率低的难题,且在校正频率方面也取得了质的飞跃。目前,系统能量利用率已从最初的5%提高到85%,基本和变形镜自适应光学系统的能量利用率相当;校正频率也从5 Hz提高到140 Hz,接近了校正大气湍流的实用化水平。利用该研究成果,分别研制了针对中科院国家天文台2.16 m望远镜和长春光机所1.2 m望远镜的液晶自适应光学系统并对恒星进行了有效校正,使1.2 m望远镜对恒星的分辨能力提高至约3倍衍射极限。
概述瞭中科院長春光學精密機械與物理研究所(長春光機所)在液晶自適應光學方麵的研究進展。針對液晶自適應光學技術存在的能量利用率低和校正頻率慢的兩大國際難題,液晶自適應光學研究組採取瞭一繫列有效措施,不但攻剋瞭能量利用率低的難題,且在校正頻率方麵也取得瞭質的飛躍。目前,繫統能量利用率已從最初的5%提高到85%,基本和變形鏡自適應光學繫統的能量利用率相噹;校正頻率也從5 Hz提高到140 Hz,接近瞭校正大氣湍流的實用化水平。利用該研究成果,分彆研製瞭針對中科院國傢天文檯2.16 m望遠鏡和長春光機所1.2 m望遠鏡的液晶自適應光學繫統併對恆星進行瞭有效校正,使1.2 m望遠鏡對恆星的分辨能力提高至約3倍衍射極限。
개술료중과원장춘광학정밀궤계여물리연구소(장춘광궤소)재액정자괄응광학방면적연구진전。침대액정자괄응광학기술존재적능량이용솔저화교정빈솔만적량대국제난제,액정자괄응광학연구조채취료일계렬유효조시,불단공극료능량이용솔저적난제,차재교정빈솔방면야취득료질적비약。목전,계통능량이용솔이종최초적5%제고도85%,기본화변형경자괄응광학계통적능량이용솔상당;교정빈솔야종5 Hz제고도140 Hz,접근료교정대기단류적실용화수평。이용해연구성과,분별연제료침대중과원국가천문태2.16 m망원경화장춘광궤소1.2 m망원경적액정자괄응광학계통병대항성진행료유효교정,사1.2 m망원경대항성적분변능력제고지약3배연사겁한。
Advances in Liquid Crystal Adaptive Optical Systems(LC AOS) are described for Changchun Institute of Optics,Fine Mechanics and Physics,Chinese Academy of Sciences(CIOMP,CAS) in this paper.For two bottlenecks of low energy utilization ratio and slow correction frequency in LC AOS problems,a series of effective methods are presented by the LC AOS working group.The low energy utilization ratio has been improved from 5% to 85%,which is similar to that of the deformable mirror based AOSs.Furthermore,the correction frequency of the LC AOS is also greatly improved from 5 Hz to 140 Hz,which is closed to the ability of correction for atmospheric turbulence.According to these research results,two LC AOSs which correspond to a 2.16 meter Telescope(located at Xinglong Station of Beijing Astronomical Observatory) and a 1.2 meter telescope(located at CIOMP,CAS) are designed to correct the stars.Obtained results show that the resolution ability of the star for the 1.2 meter telescope is up to 3 times of the diffraction limitation.