{"title":"相干自由空间激光通信的自适应接收望远镜阵列","authors":"A. Kalmar, K. Kudielka, W. Leeb","doi":"10.1364/nao.1997.mb.3","DOIUrl":null,"url":null,"abstract":"Free-space optical communication requires receive and transmit antennas in the form of telescopes. In comparison with single-aperture (“monolithic”) telescopes mainly considered so far, a phased telescope array offers many fundamental advantages: • reduced size of optical elements, • inherent modularity, therefore • redundancy (i. e. graceful degradation instead of total breakdown in case of a subtelescope failure), • reduced overall size and mass, • non-mechanical fine pointing.","PeriodicalId":135541,"journal":{"name":"Nonastronomical Adaptive Optics","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Adaptive receive telescope array for coherent free-space laser communications\",\"authors\":\"A. Kalmar, K. Kudielka, W. Leeb\",\"doi\":\"10.1364/nao.1997.mb.3\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Free-space optical communication requires receive and transmit antennas in the form of telescopes. In comparison with single-aperture (“monolithic”) telescopes mainly considered so far, a phased telescope array offers many fundamental advantages: • reduced size of optical elements, • inherent modularity, therefore • redundancy (i. e. graceful degradation instead of total breakdown in case of a subtelescope failure), • reduced overall size and mass, • non-mechanical fine pointing.\",\"PeriodicalId\":135541,\"journal\":{\"name\":\"Nonastronomical Adaptive Optics\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Nonastronomical Adaptive Optics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1364/nao.1997.mb.3\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nonastronomical Adaptive Optics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/nao.1997.mb.3","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Adaptive receive telescope array for coherent free-space laser communications
Free-space optical communication requires receive and transmit antennas in the form of telescopes. In comparison with single-aperture (“monolithic”) telescopes mainly considered so far, a phased telescope array offers many fundamental advantages: • reduced size of optical elements, • inherent modularity, therefore • redundancy (i. e. graceful degradation instead of total breakdown in case of a subtelescope failure), • reduced overall size and mass, • non-mechanical fine pointing.