{"title":"SIS接收机的高频限制","authors":"J. Zmuidzinas","doi":"10.1109/MWSYM.2015.7167149","DOIUrl":null,"url":null,"abstract":"The field of submillimeter-wavelength astronomy is blossoming thanks to major investments such as the Atacama Large Millimeter/Submillimeter Array (ALMA) and the Herschel Space Telescope. These projects were enabled by the development of very sensitive receivers, especially those using Superconductor-Insulator-Superconductor (SIS) tunnel junction diodes. Here I review some of the challenges that were faced in pushing this technology from its first demonstrations around 100 GHz to its upper frequency limit beyond 1.2 THz.","PeriodicalId":6493,"journal":{"name":"2015 IEEE MTT-S International Microwave Symposium","volume":"126 1","pages":"1-4"},"PeriodicalIF":0.0000,"publicationDate":"2015-05-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"The high-frequency limits of SIS receivers\",\"authors\":\"J. Zmuidzinas\",\"doi\":\"10.1109/MWSYM.2015.7167149\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The field of submillimeter-wavelength astronomy is blossoming thanks to major investments such as the Atacama Large Millimeter/Submillimeter Array (ALMA) and the Herschel Space Telescope. These projects were enabled by the development of very sensitive receivers, especially those using Superconductor-Insulator-Superconductor (SIS) tunnel junction diodes. Here I review some of the challenges that were faced in pushing this technology from its first demonstrations around 100 GHz to its upper frequency limit beyond 1.2 THz.\",\"PeriodicalId\":6493,\"journal\":{\"name\":\"2015 IEEE MTT-S International Microwave Symposium\",\"volume\":\"126 1\",\"pages\":\"1-4\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-05-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2015 IEEE MTT-S International Microwave Symposium\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/MWSYM.2015.7167149\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2015 IEEE MTT-S International Microwave Symposium","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/MWSYM.2015.7167149","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The field of submillimeter-wavelength astronomy is blossoming thanks to major investments such as the Atacama Large Millimeter/Submillimeter Array (ALMA) and the Herschel Space Telescope. These projects were enabled by the development of very sensitive receivers, especially those using Superconductor-Insulator-Superconductor (SIS) tunnel junction diodes. Here I review some of the challenges that were faced in pushing this technology from its first demonstrations around 100 GHz to its upper frequency limit beyond 1.2 THz.
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