A V-Band SiGe Image-Reject Receiver Front-End for Atmospheric Remote Sensing

Milad Frounchi, C. Coen, Clifford D. Y. Cheon, N. Lourenco, Wyman Williams, J. Cressler
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引用次数: 7

Abstract

This paper presents a V-band receiver front-end for spaceborne atmospheric remote sensing. The receiver is implemented in a $\mathbf{0.13}\mu\mathbf{m}$ SiGe BiCMOS technology with $f_{T}/f_{MAX}$ of 250/330 GHz and consists of a Dicke switch, an LNA, an image-reject mixer, a frequency multiplier, and an IF amplifier. Across 56–69 GHz, the receiver achieves a mean conversion gain of 65 dB, a minimum noise figure of 4.3/6.1 dB without/with the Dicke switch, and a mean image rejection ratio of 31dB. The high-gain frequency quadrupler allows operation with an LO power as low as −18 dBm. This chip consumes a total DC power of 180 mW and occupies an active area of 3.1 mm2. This is the first reported monolithic receiver front-end for atmospheric measurements across the 60 GHz oxygen spectrum and it achieves the lowest noise figure among similar Si-based Dicke radiometers.
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一种用于大气遥感的v波段SiGe图像抑制接收机前端
提出了一种用于星载大气遥感的v波段接收机前端。该接收机采用$\mathbf{0.13}\mu\mathbf{m}$ SiGe BiCMOS技术实现,$f_{T}/f_{MAX}$为250/330 GHz,由Dicke开关、LNA、图像抑制混频器、倍频器和中频放大器组成。在56-69 GHz范围内,接收机的平均转换增益为65 dB,无/带Dicke开关时的最小噪声系数为4.3/6.1 dB,平均图像抑制比为31dB。高增益频率四倍器允许工作低至- 18 dBm的LO功率。该芯片的总直流功率为180mw,有效面积为3.1 mm2。这是第一个报道的用于60 GHz氧谱大气测量的单片接收器前端,它在类似的si基Dicke辐射计中实现了最低的噪声系数。
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