R. Bohlander, V. Brady, A. Mcsweeney, G. Kirkman, J. Newton, A. Davis, O. Simpson
{"title":"一种用于测量角闪烁的准光学毫米波发射和接收阵列","authors":"R. Bohlander, V. Brady, A. Mcsweeney, G. Kirkman, J. Newton, A. Davis, O. Simpson","doi":"10.1109/IRMM.1983.9126479","DOIUrl":null,"url":null,"abstract":"This system, used to measure the effects of atmospheric turbulence at frequencies between 116 and 173 GHz, comprises a front-fed, off-axis parabola transmitting antenna located 1.4 km from a receiver array. The five antennas in the latter receive local oscillator power from a phase-locked klystron source via a low-loss lens beam waveguide distribution system.","PeriodicalId":314918,"journal":{"name":"1983 Eighth International Conference on Infrared and Millimeter Waves","volume":"102 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1983-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":"{\"title\":\"A quasi-optical millimeter wave transmitter and receiver array for measurements of angular scintillation\",\"authors\":\"R. Bohlander, V. Brady, A. Mcsweeney, G. Kirkman, J. Newton, A. Davis, O. Simpson\",\"doi\":\"10.1109/IRMM.1983.9126479\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"This system, used to measure the effects of atmospheric turbulence at frequencies between 116 and 173 GHz, comprises a front-fed, off-axis parabola transmitting antenna located 1.4 km from a receiver array. The five antennas in the latter receive local oscillator power from a phase-locked klystron source via a low-loss lens beam waveguide distribution system.\",\"PeriodicalId\":314918,\"journal\":{\"name\":\"1983 Eighth International Conference on Infrared and Millimeter Waves\",\"volume\":\"102 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1983-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"3\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"1983 Eighth International Conference on Infrared and Millimeter Waves\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/IRMM.1983.9126479\",\"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 Eighth International Conference on Infrared and Millimeter Waves","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/IRMM.1983.9126479","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A quasi-optical millimeter wave transmitter and receiver array for measurements of angular scintillation
This system, used to measure the effects of atmospheric turbulence at frequencies between 116 and 173 GHz, comprises a front-fed, off-axis parabola transmitting antenna located 1.4 km from a receiver array. The five antennas in the latter receive local oscillator power from a phase-locked klystron source via a low-loss lens beam waveguide distribution system.