{"title":"两个离轴抛物面镜在太阳物理应用中的理论分析","authors":"T. Saha, D. Leviton","doi":"10.1364/soa.1991.me1","DOIUrl":null,"url":null,"abstract":"The SUMER - Solar Ultraviolet Measurements of Emitted Radiation - instrument will be flown on the SOHO mission. The instrument will study the upper atmosphere of the sun in the 600 Å -1600 Å wavelength region. The SUMER instrument consists of an off-axis paraboloid followed by a slit, off-axis collimating paraboloid, scan mirror, grating, and a detector. The design parameters for the rectangular SUMER telescope mirror are listed in Table I.","PeriodicalId":184695,"journal":{"name":"Space Optics for Astrophysics and Earth and Planetary Remote Sensing","volume":"60 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Theoretical Analysis of Two Off-Axis Parabolic Mirrors for Solar Physics Applications\",\"authors\":\"T. Saha, D. Leviton\",\"doi\":\"10.1364/soa.1991.me1\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The SUMER - Solar Ultraviolet Measurements of Emitted Radiation - instrument will be flown on the SOHO mission. The instrument will study the upper atmosphere of the sun in the 600 Å -1600 Å wavelength region. The SUMER instrument consists of an off-axis paraboloid followed by a slit, off-axis collimating paraboloid, scan mirror, grating, and a detector. The design parameters for the rectangular SUMER telescope mirror are listed in Table I.\",\"PeriodicalId\":184695,\"journal\":{\"name\":\"Space Optics for Astrophysics and Earth and Planetary Remote Sensing\",\"volume\":\"60 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.me1\",\"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.me1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
摘要
太阳紫外线发射辐射测量仪器将在SOHO任务中飞行。该仪器将研究600 Å -1600 Å波长区域的太阳高层大气。SUMER仪器由一个离轴抛物面和一个狭缝、离轴准直抛物面、扫描镜、光栅和一个探测器组成。SUMER矩形望远镜反射镜的设计参数见表1。
Theoretical Analysis of Two Off-Axis Parabolic Mirrors for Solar Physics Applications
The SUMER - Solar Ultraviolet Measurements of Emitted Radiation - instrument will be flown on the SOHO mission. The instrument will study the upper atmosphere of the sun in the 600 Å -1600 Å wavelength region. The SUMER instrument consists of an off-axis paraboloid followed by a slit, off-axis collimating paraboloid, scan mirror, grating, and a detector. The design parameters for the rectangular SUMER telescope mirror are listed in Table I.
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