A 2.2 GS/s 188mW spectrometer processor in 65nm CMOS for supporting low-power THz planetary instruments

F. Hsiao, A. Tang, Y. Kim, B. Drouin, G. Chattopadhyay, Mau-Chung Frank Chang
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引用次数: 18

Abstract

The paper presents a 2.2 GS/s (1.1 GHz Nyquist bandwidth), 188 mW 512-channel spectrometer processor developed to support of future science observations on NASA planetary missions, where payload size, weight, and power consumption are extremely limited. The presented spectrometer processor chip contains a pair of 7 bit ADC IQ converters coupled with a 512 point PSD processor, and averaging accumulator, allowing it to be sensitive enough to detect trace gases like NH3, HCN, and CO2 when coupled to the appropriate band RF front-end receiver. The bandwidth and resolution of the presented processor make it suitable for exploring the composition of planets, moons and their atmospheres throughout our solar system.
一个2.2 GS/s 188mW的65纳米CMOS光谱仪处理器,支持低功耗太赫兹行星仪器
本文介绍了一种2.2 GS/s (1.1 GHz奈奎斯特带宽)、188 mW 512通道光谱仪处理器,用于支持NASA行星任务中未来的科学观测,这些任务的有效载荷大小、重量和功耗都非常有限。所提出的光谱仪处理器芯片包含一对7位ADC IQ转换器和一个512点PSD处理器,以及平均累加器,当耦合到适当频段的射频前端接收器时,使其能够足够灵敏地检测微量气体,如NH3, HCN和CO2。所展示的处理器的带宽和分辨率使其适合探索整个太阳系的行星、卫星及其大气的组成。
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