用于射电天文学的低噪声ka波段放大器

M. McCulloch, E. Blackhurst, R. Davis, A. Galtress, D. George, S. Melhuish, L. Piccirillo
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引用次数: 3

摘要

本文介绍了一种基于微波集成电路(MICs)和单片微波集成电路(mmic)杂交的低温ka波段低噪声放大器(LNA)原型的设计和结果。所得到的晶体管加上MMIC (T+MMIC) 5级LNA,峰值增益为52dB,在≈23K的环境温度下最小噪声温度为12K,带宽为27-33GHz,为20%。我们概述了LNA背后的背景,我们的测量过程,LNA的性能,我们未来的发展计划,并讨论了这种放大器布局可能提供的优势。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A low noise Ka-band amplifier for radio astronomy
We present the designs for and the results of a prototype cryogenic Ka-band low noise amplifier (LNA), that is based on the hybridization of microwave integrated circuits (MICs) and monolithic microwave integrated circuits (MMICs). The resulting transistor plus MMIC (T+MMIC) 5 stage LNA, has a peak gain of 52dB, a minimum noise temperature of 12K at an ambient temperature of ≈23K, and a 20% bandwidth of 27-33GHz. We outline the background behind the LNA, our measurement process, the LNA's performance, our future development plans and discuss the possible advantages that this amplifier layout may offer.
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