用于射电天文学的4-12 GHz和25-34 GHz低温MHEMT MMIC低噪声放大器

B. Aja, M. Seelmann-Eggebert, A. Leuther, H. Massler, M. Schlechtweg, J. Gallego, I. López-Fernández, C. Diez, I. Malo, E. Villa, E. Artal
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引用次数: 15

摘要

应用于射电天文应用的MMIC宽带低噪声放大器(LNA)采用了100 nm GaAs高电子迁移率晶体管(mHEMT)工艺。介绍了4-12 GHz和25-34 GHz LNAs的低温性能。在15 K下冷却的4-12 GHz LNA的相关增益为31.5 dB±1.8 dB,平均噪声温度为5.3 K,功耗低至8 mW。冷却至15 K时,25-34 GHz放大器的平坦增益为24.2 dB±0.4 dB,平均噪声温度为15.2 K,芯片上功耗极低,仅为2.8 mW。基于mHEMT的LNA mmic在低温下表现出优异的噪声特性,可用于射电天文学应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
4–12 GHz and 25–34 GHz cryogenic MHEMT MMIC Low Noise Amplifiers for radio astronomy
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorphic High Electron Mobility Transistor (mHEMT) process have been developed. Cryogenic performance of a 4–12 GHz and a 25–34 GHz LNAs is presented. The 4–12 GHz LNA cooled at 15 K exhibits an associated gain of 31.5 dB ± 1.8 dB and average noise temperature of 5.3 K with a low power dissipation of 8 mW. Cooled to 15 K the 25–34 GHz amplifier has demonstrated a flat gain of 24.2 dB ± 0.4 dB with 15.2 K average noise temperature, and a very low power dissipation of 2.8 mW on chip. The mHEMT based LNA MMICs have demonstrated excellent noise characteristics at cryogenic temperatures for their use in radio astronomy applications.
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