4–12 GHz and 25–34 GHz cryogenic MHEMT MMIC Low Noise Amplifiers for radio astronomy

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

Abstract

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.
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
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。
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