{"title":"HST模拟器零功率校正器的光学设计","authors":"P. Davila, P. G. Hannan","doi":"10.1364/soa.1991.tue1","DOIUrl":null,"url":null,"abstract":"Images from the Hubble Space Telescope (HST) suffer from overcorrected spherical aberration1. The optical designs of the second generation instruments, such as the Wide Field/Planetary Camera (WFPC-2), the Space Telescope Imaging Spectrograph (STIS), and the Near Infrared Camera (NIC), are being modified to correct or compensate the spherical aberration of the HST.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"201 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Optical Design of a Zero Power Corrector for HST Simulators\",\"authors\":\"P. Davila, P. G. Hannan\",\"doi\":\"10.1364/soa.1991.tue1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Images from the Hubble Space Telescope (HST) suffer from overcorrected spherical aberration1. The optical designs of the second generation instruments, such as the Wide Field/Planetary Camera (WFPC-2), the Space Telescope Imaging Spectrograph (STIS), and the Near Infrared Camera (NIC), are being modified to correct or compensate the spherical aberration of the HST.\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"201 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.1991.tue1\",\"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.1991.tue1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Optical Design of a Zero Power Corrector for HST Simulators
Images from the Hubble Space Telescope (HST) suffer from overcorrected spherical aberration1. The optical designs of the second generation instruments, such as the Wide Field/Planetary Camera (WFPC-2), the Space Telescope Imaging Spectrograph (STIS), and the Near Infrared Camera (NIC), are being modified to correct or compensate the spherical aberration of the HST.