{"title":"光纤连接光学望远镜阵列(浮子)","authors":"P. Connes","doi":"10.1364/soa.1988.wb8","DOIUrl":null,"url":null,"abstract":"We will describe the space version of our FLOAT proposal. This will be an array of telescopes connected by equal-length single-mode fibers to a mixing station, where the images will be synthesized. The main advantage, compared to all-mirror proposals, is a large simplification of the adjustment problem; the main limitation is exclsuion of far UV. A first step will be a similar array built on a ground-based radiotelescope.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"3 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Fiber-Linked Optical Array of Telescopes (FLOAT)\",\"authors\":\"P. Connes\",\"doi\":\"10.1364/soa.1988.wb8\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We will describe the space version of our FLOAT proposal. This will be an array of telescopes connected by equal-length single-mode fibers to a mixing station, where the images will be synthesized. The main advantage, compared to all-mirror proposals, is a large simplification of the adjustment problem; the main limitation is exclsuion of far UV. A first step will be a similar array built on a ground-based radiotelescope.\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"3 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.wb8\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","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.wb8","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
We will describe the space version of our FLOAT proposal. This will be an array of telescopes connected by equal-length single-mode fibers to a mixing station, where the images will be synthesized. The main advantage, compared to all-mirror proposals, is a large simplification of the adjustment problem; the main limitation is exclsuion of far UV. A first step will be a similar array built on a ground-based radiotelescope.
求助内容：
应助结果提醒方式：
京公网安备 11010802042870号
