{"title":"用于空间的入门级干涉仪","authors":"P. Bely, C. Burrows, F. Roddier, G. Weigelt","doi":"10.1364/soa.1988.tua5","DOIUrl":null,"url":null,"abstract":"Observational optical astronomy is always scientifically driven to develop telescopes with fainter limiting magnitude and higher resolution. Larger ground-based telescopes are more sensitive, but give little improvement in resolution unless extremely demanding interferometric techniques are used. Space-based telescopes of traditional configuration such as the Hubble Space Telescope (HST) give great improvements in resolution being diffraction limited, and a consequent improvement in limiting magnitude, but further improvements are limited by launch constraints.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"5 5 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"An Entry Level Interferometer for Space\",\"authors\":\"P. Bely, C. Burrows, F. Roddier, G. Weigelt\",\"doi\":\"10.1364/soa.1988.tua5\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Observational optical astronomy is always scientifically driven to develop telescopes with fainter limiting magnitude and higher resolution. Larger ground-based telescopes are more sensitive, but give little improvement in resolution unless extremely demanding interferometric techniques are used. Space-based telescopes of traditional configuration such as the Hubble Space Telescope (HST) give great improvements in resolution being diffraction limited, and a consequent improvement in limiting magnitude, but further improvements are limited by launch constraints.\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"5 5 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.tua5\",\"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.tua5","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Observational optical astronomy is always scientifically driven to develop telescopes with fainter limiting magnitude and higher resolution. Larger ground-based telescopes are more sensitive, but give little improvement in resolution unless extremely demanding interferometric techniques are used. Space-based telescopes of traditional configuration such as the Hubble Space Telescope (HST) give great improvements in resolution being diffraction limited, and a consequent improvement in limiting magnitude, but further improvements are limited by launch constraints.