A Four Telescope Wide Field of View Phased Array

C. R. De Hainaut, K. Hentz, L. D. Weaver, J. Gonglewski
{"title":"A Four Telescope Wide Field of View Phased Array","authors":"C. R. De Hainaut, K. Hentz, L. D. Weaver, J. Gonglewski","doi":"10.1364/soa.1988.wb11","DOIUrl":null,"url":null,"abstract":"A phased array telescope is an array of optical telescopes whose images are coherently combined so as to achieve the resolution of a single but much larger telescope. Design of a wide field of view phased array imaging system is considerably more difficult than phased array beam transmission telescopes such as PHASAR,1 which has no field of view. In addition to maintaining optical phase to a fraction of a wavelength on the optic axis, an imaging telescope must accurately control phase and align the images from all telescopes to within a fraction of a resolution element over the whole field of view simultaneously. This requires lateral pupil geometry3 that is extremely close to the ideal.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"47 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/soa.1988.wb11","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

A phased array telescope is an array of optical telescopes whose images are coherently combined so as to achieve the resolution of a single but much larger telescope. Design of a wide field of view phased array imaging system is considerably more difficult than phased array beam transmission telescopes such as PHASAR,1 which has no field of view. In addition to maintaining optical phase to a fraction of a wavelength on the optic axis, an imaging telescope must accurately control phase and align the images from all telescopes to within a fraction of a resolution element over the whole field of view simultaneously. This requires lateral pupil geometry3 that is extremely close to the ideal.
四望远镜宽视场相控阵
相控阵望远镜是一组光学望远镜,它们的图像被相干地组合在一起,以达到单个但更大的望远镜的分辨率。宽视场相控阵成像系统的设计要比无视场的相控阵波束传输望远镜(如PHASAR 1)困难得多。除了将光学相位保持在光轴上波长的一小部分之外,成像望远镜还必须精确地控制相位,并将来自所有望远镜的图像同时对准整个视场的分辨率元素的一小部分。这就要求侧瞳几何极为接近理想。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信