6.5-45.5GHz超宽带致冷接收机的关键技术研究

致冷接收机是射电天文望远镜的核心观测设备，更低的噪声和更宽的观测频带是接收机技术一直追寻的两大发展目标。本项目首次提出研究覆盖厘米波段至长毫米波波段的超宽带致冷接收机，频率范围6.5-45.5GHz，包含C/X/Ku/K/Ka/Q共计六个射电天文波段，含馈源在内的接收机整体噪声温度低于40K，可以开展超过30条重要天文谱线观测、超过30GHz带宽天文连续谱观测、实现C/K/Q和X/Ka等灵活的多波段组合观测。本项目将针对四项关键技术开展研究，超宽带馈源和极化器为核心的无源器件研究、超宽带致冷MMIC低噪声放大器为核心的有源器件研究、大口径低损耗微波窗口为核心的整体致冷技术研究、高镜像抑制和宽带频率合成为核心的超宽带变频技术研究。6.5-45.5GHz超宽带致冷接收机适用于主焦和卡焦类型的抛物面天线，将为厘米波段射电望远镜及其阵列提供全新的观测视角，多波段同时观测数据将支撑未知的科学发现。

Cryogenic receiver is the most important equipment on the radio astronomical telescope. Lower noise and wider bandwidth are big goals for radio astronomy receiver technology development. The research target is building the ultra-wideband cryogenic receiver which has observation frequency range of 6.5 GHz to 45.5 GHz, could cover C/X/Ku/K/Ka/Q for a total six radio astronomy bands. The receiver noise temperature could be less than 40 Kelvin by cooling the whole feed and LNAs. Many flexible applications can be carried out, including more than 30 major spectral lines observation, more than 30 GHz bandwidth continuum spectrum observation, such as C/K/Q or X/Ka multiband observation. This project will focus on four key technologies, the ultra-wideband feed horn and polarizer, ultra-wideband cryogenic MMIC low noise amplifier, the large size low loss microwave vacuum window, the broadband high image reject converter and powerful synthesizer. The 6.5-45.5 GHz ultra-wide cryogenic receiver could be suitable for applications either main focus or second focus of the parabolic antenna. The receiver will provide a new observation window for the large scale single dish telescopes and array which are working at centimeter wavelength. The multi-band simultaneous observation data will provide opportunities for more scientific discoveries.