Xi Fu, Yun Wang, Dongwon You, Xiaolin Wang, A. Fadila, Yi Zhang, Sena Kato, Chun Wang, Zheng Li, Jian Pang, A. Shirane, K. Okada
{"title":"基于磁调谐移相器的3.4mW/元抗辐射ka波段CMOS相控阵接收机","authors":"Xi Fu, Yun Wang, Dongwon You, Xiaolin Wang, A. Fadila, Yi Zhang, Sena Kato, Chun Wang, Zheng Li, Jian Pang, A. Shirane, K. Okada","doi":"10.1109/ISSCC42614.2022.9731557","DOIUrl":null,"url":null,"abstract":"Low-Earth-Orbit (LEO) satellite constellations have been demonstrated as a ground breaking technology for providing low-cost low-latency global internet access. However, each satellite needs more than 200kg launch mass due to bulky wireless components and solar cells, which raises a serious cost issue. One possible solution is further minimizing satellite mass, such as cube satellites, by realizing an ultra-low-power Kaband phased-array transceiver. In this work, 1W power consumption is targeted for a 256-element Ka-band phased-array receiver, i.e. 4mW per element. In the conventional geostationary communication satellites, a parabolic antenna is utilized, and a transceiver module is placed inside a metallic cavity so it can tolerate cosmic radiation. On the other hand, LEO satellites need beam-steering functionality by using a phased-array antenna, and only a thin shield layer can be inserted between antennas and ICs for avoiding redundant mass and insertion loss. Thus, the radiation-hardening and low power consumption are key requirements for such cube satellite phased arrays. For RF building blocks in a phased array, the total ionizing dose (TID) is more critical than the single event effects (SEE). Figure 4.8.1 shows an estimated result for non-radiation-hardened design regarding TID degradation on beam pattern, resulting in 3.8dB main-lobe degradation. In this work, 2.7Mrad TID tolerance is considered adequate for a 3-year lifespan with a 24pm PCB copper shield. Figure 4.8.1 also summarizes the system requirements for a phased-array satellite receiver.","PeriodicalId":6830,"journal":{"name":"2022 IEEE International Solid- State Circuits Conference (ISSCC)","volume":"6 1","pages":"90-92"},"PeriodicalIF":0.0000,"publicationDate":"2022-02-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"6","resultStr":"{\"title\":\"A 3.4mW/element Radiation-Hardened Ka-Band CMOS Phased-Array Receiver Utilizing Magnetic-Tuning Phase Shifter for Small Satellite Constellation\",\"authors\":\"Xi Fu, Yun Wang, Dongwon You, Xiaolin Wang, A. Fadila, Yi Zhang, Sena Kato, Chun Wang, Zheng Li, Jian Pang, A. Shirane, K. Okada\",\"doi\":\"10.1109/ISSCC42614.2022.9731557\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Low-Earth-Orbit (LEO) satellite constellations have been demonstrated as a ground breaking technology for providing low-cost low-latency global internet access. However, each satellite needs more than 200kg launch mass due to bulky wireless components and solar cells, which raises a serious cost issue. One possible solution is further minimizing satellite mass, such as cube satellites, by realizing an ultra-low-power Kaband phased-array transceiver. In this work, 1W power consumption is targeted for a 256-element Ka-band phased-array receiver, i.e. 4mW per element. In the conventional geostationary communication satellites, a parabolic antenna is utilized, and a transceiver module is placed inside a metallic cavity so it can tolerate cosmic radiation. On the other hand, LEO satellites need beam-steering functionality by using a phased-array antenna, and only a thin shield layer can be inserted between antennas and ICs for avoiding redundant mass and insertion loss. Thus, the radiation-hardening and low power consumption are key requirements for such cube satellite phased arrays. For RF building blocks in a phased array, the total ionizing dose (TID) is more critical than the single event effects (SEE). Figure 4.8.1 shows an estimated result for non-radiation-hardened design regarding TID degradation on beam pattern, resulting in 3.8dB main-lobe degradation. In this work, 2.7Mrad TID tolerance is considered adequate for a 3-year lifespan with a 24pm PCB copper shield. Figure 4.8.1 also summarizes the system requirements for a phased-array satellite receiver.\",\"PeriodicalId\":6830,\"journal\":{\"name\":\"2022 IEEE International Solid- State Circuits Conference (ISSCC)\",\"volume\":\"6 1\",\"pages\":\"90-92\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2022-02-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"6\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2022 IEEE International Solid- State Circuits Conference (ISSCC)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/ISSCC42614.2022.9731557\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2022 IEEE International Solid- State Circuits Conference (ISSCC)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ISSCC42614.2022.9731557","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A 3.4mW/element Radiation-Hardened Ka-Band CMOS Phased-Array Receiver Utilizing Magnetic-Tuning Phase Shifter for Small Satellite Constellation
Low-Earth-Orbit (LEO) satellite constellations have been demonstrated as a ground breaking technology for providing low-cost low-latency global internet access. However, each satellite needs more than 200kg launch mass due to bulky wireless components and solar cells, which raises a serious cost issue. One possible solution is further minimizing satellite mass, such as cube satellites, by realizing an ultra-low-power Kaband phased-array transceiver. In this work, 1W power consumption is targeted for a 256-element Ka-band phased-array receiver, i.e. 4mW per element. In the conventional geostationary communication satellites, a parabolic antenna is utilized, and a transceiver module is placed inside a metallic cavity so it can tolerate cosmic radiation. On the other hand, LEO satellites need beam-steering functionality by using a phased-array antenna, and only a thin shield layer can be inserted between antennas and ICs for avoiding redundant mass and insertion loss. Thus, the radiation-hardening and low power consumption are key requirements for such cube satellite phased arrays. For RF building blocks in a phased array, the total ionizing dose (TID) is more critical than the single event effects (SEE). Figure 4.8.1 shows an estimated result for non-radiation-hardened design regarding TID degradation on beam pattern, resulting in 3.8dB main-lobe degradation. In this work, 2.7Mrad TID tolerance is considered adequate for a 3-year lifespan with a 24pm PCB copper shield. Figure 4.8.1 also summarizes the system requirements for a phased-array satellite receiver.