{"title":"莱曼光学，远紫外光谱探测器","authors":"W. Cash","doi":"10.1364/soa.1988.tuc3","DOIUrl":null,"url":null,"abstract":"Lyman, the Far Ultraviolet Explorer, is a space astrophysics mission designed to explore the spectra of celestial sources in the ultraviolet from 100 to 1250Å, the gap between the Hubble Space Telescope and the Advanced X-ray Astrophysics Facility. Lyman was recently selected by NASA as one of four missions to enter Phase A studies with a goal of launch in the mid-1990’s. It is envisioned as a community observatory in the tradition of the International Ultraviolet Explorer.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Optics for Lyman, The Far Ultraviolet Spectroscopic Explorer\",\"authors\":\"W. Cash\",\"doi\":\"10.1364/soa.1988.tuc3\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Lyman, the Far Ultraviolet Explorer, is a space astrophysics mission designed to explore the spectra of celestial sources in the ultraviolet from 100 to 1250Å, the gap between the Hubble Space Telescope and the Advanced X-ray Astrophysics Facility. Lyman was recently selected by NASA as one of four missions to enter Phase A studies with a goal of launch in the mid-1990’s. It is envisioned as a community observatory in the tradition of the International Ultraviolet Explorer.\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"1 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.tuc3\",\"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.tuc3","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Optics for Lyman, The Far Ultraviolet Spectroscopic Explorer
Lyman, the Far Ultraviolet Explorer, is a space astrophysics mission designed to explore the spectra of celestial sources in the ultraviolet from 100 to 1250Å, the gap between the Hubble Space Telescope and the Advanced X-ray Astrophysics Facility. Lyman was recently selected by NASA as one of four missions to enter Phase A studies with a goal of launch in the mid-1990’s. It is envisioned as a community observatory in the tradition of the International Ultraviolet Explorer.
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