{"title":"空间阵列望远镜的一阶光学设计考虑","authors":"E. Hochberg, N. Page","doi":"10.1364/soa.1988.wb9","DOIUrl":null,"url":null,"abstract":"For the purpose of comparing the various optical design approaches for a space-based array telescope, the following performance goals will be used: The UV operational goal is motivated by the desire to obtain information inaccessible to the ground based astronomer while the 30 meter baseline obtains from the desire for milliarc-second class angular resolution;","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"38 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"First-Order Optical Design Considerations for Spaced-Based Array Telescopes\",\"authors\":\"E. Hochberg, N. Page\",\"doi\":\"10.1364/soa.1988.wb9\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"For the purpose of comparing the various optical design approaches for a space-based array telescope, the following performance goals will be used: The UV operational goal is motivated by the desire to obtain information inaccessible to the ground based astronomer while the 30 meter baseline obtains from the desire for milliarc-second class angular resolution;\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"38 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.wb9\",\"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.wb9","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
First-Order Optical Design Considerations for Spaced-Based Array Telescopes
For the purpose of comparing the various optical design approaches for a space-based array telescope, the following performance goals will be used: The UV operational goal is motivated by the desire to obtain information inaccessible to the ground based astronomer while the 30 meter baseline obtains from the desire for milliarc-second class angular resolution;