Wideband W-Band GAN LNA MMIC with State-of-the-Art Noise Figure

S. Lardizabal, K. C. Hwang, J. Kotce, A. Brown, A. Fung
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引用次数: 22

Abstract

W-band GaN amplifiers developed for the NASA Earth Science Technology Office, ESTO, enable compact active electronically steerable arrays (AESA's) for cloud Doppler radar. This paper describes the design fabrication and test of 100 nm GaN HEMT low noise amplifiers for NASA's latest 3-band Doppler radar instrument concept. Our results show state-of-the-art performance for a 92 GHz to 96 GHz channel with gain greater than 17 dB and noise figure less than 5 dB. Detailed on-wafer testing shows record low measured noise figure of 3.0 dB with 20 dB of gain and dc power of 128 mW using a 5 Volt supply.
具有最先进噪声图的宽带w波段GAN LNA MMIC
为NASA地球科学技术办公室(ESTO)开发的w波段GaN放大器,可为云多普勒雷达提供紧凑型有源电子制导阵列(AESA)。本文介绍了NASA最新3波段多普勒雷达仪器概念中100nm GaN HEMT低噪声放大器的设计、制造和测试。我们的研究结果显示,在92 GHz至96 GHz信道上,增益大于17 dB,噪声系数小于5 dB,具有最先进的性能。详细的晶圆上测试显示,在5伏电源下,增益为20 dB,直流功率为128 mW的情况下,测量到的噪声指数达到创纪录的3.0 dB。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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