Performance modeling of the adaptive optics system on the 2.16 m telescope
The adaptive optics system on the 2.16 m telescope is modeled and simulated using an ends-to-ends Monte Carlo method in this paper. Under the optimized parameters, the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J, H and K bands with a classical adaptive optics system. Base...
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Veröffentlicht in: | 中国科学:化学英文版 2013 (3), p.658-662 |
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description | The adaptive optics system on the 2.16 m telescope is modeled and simulated using an ends-to-ends Monte Carlo method in this paper. Under the optimized parameters, the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J, H and K bands with a classical adaptive optics system. Based on the simulation results, the practical system design is also considered and discussed. |
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Under the optimized parameters, the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J, H and K bands with a classical adaptive optics system. 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Based on the simulation results, the practical system design is also considered and discussed.</description><subject>Strehl比</subject><subject>仿真结果</subject><subject>实际系统</subject><subject>性能建模</subject><subject>望远镜</subject><subject>自适应光学系统</subject><issn>1674-7291</issn><issn>1869-1870</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqNjE0KwjAUhIMoWLR3eB6g0rQxadeiiCsX7iWkrz_SJDUJQm9vEA_gbL6Bb5gFSWjF64xWIl_GzgXLRFHTNUm9f-YxZZkX4pCQ6w1da52WRiFo2-A4mA5sC6FHkI2cwvBGsBHKg599QA3WfG2xpxw0BBzRKzvhlqxaOXpMf9yQ3fl0P14y1VvTveLvY3KDlm5-MCZ4zaqq_GfzAf8MPMc</recordid><startdate>2013</startdate><enddate>2013</enddate><creator>JIA Peng ZHANG SiJiong</creator><scope>2RA</scope><scope>92L</scope><scope>CQIGP</scope><scope>~WA</scope></search><sort><creationdate>2013</creationdate><title>Performance modeling of the adaptive optics system on the 2.16 m telescope</title><author>JIA Peng ZHANG SiJiong</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-chongqing_primary_447694883</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Strehl比</topic><topic>仿真结果</topic><topic>实际系统</topic><topic>性能建模</topic><topic>望远镜</topic><topic>自适应光学系统</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>JIA Peng ZHANG SiJiong</creatorcontrib><collection>中文科技期刊数据库</collection><collection>中文科技期刊数据库-CALIS站点</collection><collection>中文科技期刊数据库-7.0平台</collection><collection>中文科技期刊数据库- 镜像站点</collection><jtitle>中国科学:化学英文版</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>JIA Peng ZHANG SiJiong</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Performance modeling of the adaptive optics system on the 2.16 m telescope</atitle><jtitle>中国科学:化学英文版</jtitle><addtitle>SCIENCE CHINA Chemistry</addtitle><date>2013</date><risdate>2013</risdate><issue>3</issue><spage>658</spage><epage>662</epage><pages>658-662</pages><issn>1674-7291</issn><eissn>1869-1870</eissn><abstract>The adaptive optics system on the 2.16 m telescope is modeled and simulated using an ends-to-ends Monte Carlo method in this paper. Under the optimized parameters, the Strehl ratio can be increased from about 0.02 to more than 0.2 in the J, H and K bands with a classical adaptive optics system. Based on the simulation results, the practical system design is also considered and discussed.</abstract></addata></record> |
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issn | 1674-7291 1869-1870 |
language | eng |
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source | SpringerLink Journals; Alma/SFX Local Collection; ProQuest Central |
subjects | Strehl比 仿真结果 实际系统 性能建模 望远镜 自适应光学系统 |
title | Performance modeling of the adaptive optics system on the 2.16 m telescope |
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