⚡ 本页包含 AI 生成的分析内容,仅供参考
该论文提出了一款210至305GHz的CMOS接收机前端,用于旋转光谱学中的气体分子检测。通过集成片上天线并采用相位补偿人工磁导体(PC-AMC)替代金属反射器,实现了13.9至19dB的单边带噪声系数。
sub-millimeter-wave frequency ranges are used in fast-scan rotational spectroscopy to detect gas molecules and measure their concentrations [1]. This technique can be used for indoor air quality monitoring, detection of toxic gas leaks, breath analyses for monitoring bodily conditions and many others. This paper reports a 210-to-305GHz receiver (RX) front-end for a rotational spectrometer that achieves SSB noise figure (NF) of 13.9 to 19dB by incorporating an on-chip antenna with a reflector formed using a phase-compensated artificial magnetic conductor (PC-AMC) instead a metal reflector to improve the bandwidth of the antenna, a single balanced subharmonic mixer using a pair of floating-body NMOS anti-parallel diode pairs (FB-APDPs), a hybrid-based broadband port-isolation structure, and a 20-GHz low-noise
Qian Zhong, Wooyeol Choi, Christopher Miller,
Rashaunda Henderson, Kenneth K O University of Texas, Dallas, TX Electromagnetic waves in the millimeter- and