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Low-noise 0.8-0.96- and 0.96-1.12-THz superconductor-insulator-superconductor mixers for the Herschel Space Observatory

机译:赫歇尔天文台的低噪声0.8-0.96-和0.96-1.12-THz超导体-绝缘体-超导体混合器

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摘要

Heterodyne mixers incorporating Nb SIS junctions and NbTiN-SiO/sub 2/-Al microstrip tuning circuits offer the lowest reported receiver noise temperatures to date in the 0.8-0.96- and 0.96-1.12-THz frequency bands. In particular, improvements in the quality of the NbTiN ground plane of the SIS devices' on-chip microstrip tuning circuits have yielded significant improvements in the sensitivity of the 0.96-1.12-THz mixers relative to previously presented results. Additionally, an optimized RF design incorporating a reduced-height waveguide and suspended stripline RF choke filter offers significantly larger operating bandwidths than were obtained with mixers that incorporated full-height waveguides near 1 THz. Finally, the impact of junction current density and quality on the performance of the 0.8-0.96-THz mixers is discussed and compared with measured mixer sensitivities, as are the relative sensitivities of the 0.8-0.96- and 0.96-1.12-THz mixers.
机译:包含Nb SIS结和NbTiN-SiO / sub 2 / -Al微带调谐电路的外差混频器在0.8-0.96-和0.96-1.12-THz频带中提供了迄今为止最低的接收机噪声温度。尤其是,SIS器件的片上微带调谐电路的NbTiN接地层质量的提高相对于先前提出的结果,已经大大提高了0.96-1.12-THz混频器的灵敏度。此外,结合了高度减小的波导和悬浮带状线RF扼流滤波器的优化RF设计比结合了1 THz附近的全高度波导的混频器提供了更大的工作带宽。最后,讨论了结电流密度和质量对0.8-0.96-THz混频器性能的影响,并将其与测得的混频器灵敏度进行了比较,以及0.8-0.96-和0.96-1.12-THz混频器的相对灵敏度。

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