{"title":"用于毫米波和亚毫米波天文观测的精密3米射电望远镜","authors":"B. Vowinkel, G. Winnewisser, H. Mader, W. Pritzer","doi":"10.1109/EUMA.1983.333191","DOIUrl":null,"url":null,"abstract":"A 3-m Radiotelescope with a surface accuracy of 30¿m (r.m.s.) has been constructed that will be used for astronomical observations at millimeter and sub-millimeter wavelengths. At present the telescope is equipped with a tunable receiver for the frequency range from 80 to 90 GHz, a 256-channel filter spectrometer and an acousto-optic high resolution spectrometer. The various telescope and receiver control functions are carried out by micro-processors, controlled by a POP 11/34 computer.","PeriodicalId":105436,"journal":{"name":"1983 13th European Microwave Conference","volume":"133 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1983-09-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A Precision 3-m Radiotelescope for Astronomical Observations at Millimeter and Sub-Millimeter Wavelengths\",\"authors\":\"B. Vowinkel, G. Winnewisser, H. Mader, W. Pritzer\",\"doi\":\"10.1109/EUMA.1983.333191\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A 3-m Radiotelescope with a surface accuracy of 30¿m (r.m.s.) has been constructed that will be used for astronomical observations at millimeter and sub-millimeter wavelengths. At present the telescope is equipped with a tunable receiver for the frequency range from 80 to 90 GHz, a 256-channel filter spectrometer and an acousto-optic high resolution spectrometer. The various telescope and receiver control functions are carried out by micro-processors, controlled by a POP 11/34 computer.\",\"PeriodicalId\":105436,\"journal\":{\"name\":\"1983 13th European Microwave Conference\",\"volume\":\"133 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1983-09-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"1983 13th European Microwave Conference\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/EUMA.1983.333191\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"1983 13th European Microwave Conference","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/EUMA.1983.333191","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A Precision 3-m Radiotelescope for Astronomical Observations at Millimeter and Sub-Millimeter Wavelengths
A 3-m Radiotelescope with a surface accuracy of 30¿m (r.m.s.) has been constructed that will be used for astronomical observations at millimeter and sub-millimeter wavelengths. At present the telescope is equipped with a tunable receiver for the frequency range from 80 to 90 GHz, a 256-channel filter spectrometer and an acousto-optic high resolution spectrometer. The various telescope and receiver control functions are carried out by micro-processors, controlled by a POP 11/34 computer.
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