{"title":"一种新型毫米波SIS混频器,包括串联结阵列和片上偏置- t","authors":"Wentao Wu, W. Shan","doi":"10.1109/APMC.2015.7413443","DOIUrl":null,"url":null,"abstract":"In this paper, we introduce a novel Superconductor-Insulator-Superconductor (SIS) mixer circuitry based on a series-connected junction (SJ) array. Unlike existing SJ designs, in which each junction is biased at the same DC current. This new design enables each junction to be DC-biased at the same voltage via a set of on-chip bias-T's. Thanks to this parallel DC biasing solution, this circuit design supports a so-called series-connected distributed junction (SDJ) array design, in which LO power non-uniformly spreads along the junction array both in amplitude and in phase. Using this SDJ array, we can realize mm-wave SIS mixers with octave RF band, 15 GHz-wide IF band and high dynamic range required for radio astronomical observation. Simulations of an 80-160GHz SIS mixer design have been made based on this design to support our arguments.","PeriodicalId":269888,"journal":{"name":"2015 Asia-Pacific Microwave Conference (APMC)","volume":"29 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2015-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"A novel mm-wave SIS mixer comprising series-connected junction array and on-chip bias-T\",\"authors\":\"Wentao Wu, W. Shan\",\"doi\":\"10.1109/APMC.2015.7413443\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this paper, we introduce a novel Superconductor-Insulator-Superconductor (SIS) mixer circuitry based on a series-connected junction (SJ) array. Unlike existing SJ designs, in which each junction is biased at the same DC current. This new design enables each junction to be DC-biased at the same voltage via a set of on-chip bias-T's. Thanks to this parallel DC biasing solution, this circuit design supports a so-called series-connected distributed junction (SDJ) array design, in which LO power non-uniformly spreads along the junction array both in amplitude and in phase. Using this SDJ array, we can realize mm-wave SIS mixers with octave RF band, 15 GHz-wide IF band and high dynamic range required for radio astronomical observation. Simulations of an 80-160GHz SIS mixer design have been made based on this design to support our arguments.\",\"PeriodicalId\":269888,\"journal\":{\"name\":\"2015 Asia-Pacific Microwave Conference (APMC)\",\"volume\":\"29 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2015-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2015 Asia-Pacific Microwave Conference (APMC)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/APMC.2015.7413443\",\"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 Asia-Pacific Microwave Conference (APMC)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/APMC.2015.7413443","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A novel mm-wave SIS mixer comprising series-connected junction array and on-chip bias-T
In this paper, we introduce a novel Superconductor-Insulator-Superconductor (SIS) mixer circuitry based on a series-connected junction (SJ) array. Unlike existing SJ designs, in which each junction is biased at the same DC current. This new design enables each junction to be DC-biased at the same voltage via a set of on-chip bias-T's. Thanks to this parallel DC biasing solution, this circuit design supports a so-called series-connected distributed junction (SDJ) array design, in which LO power non-uniformly spreads along the junction array both in amplitude and in phase. Using this SDJ array, we can realize mm-wave SIS mixers with octave RF band, 15 GHz-wide IF band and high dynamic range required for radio astronomical observation. Simulations of an 80-160GHz SIS mixer design have been made based on this design to support our arguments.