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Broadband Differential Low-Noise Amplifier for Active Differential Arrays

机译:有源差分阵列宽带差分低噪声放大器

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摘要

In this paper, differential low-noise amplifiers are presented as a very powerful solution for radio astronomy applications. A fully differential amplifier topology has been analyzed and implemented in microstrip technology with discrete surface mount components. The amplifier design is made for an active receiving dense antenna array. Thus, the differential amplifier source impedance is no longer 50 $Omega$ , but 150 $Omega$ from the proposed bunny-ear antennas. A full characterization in terms of gain and noise has been undertaken. Source–pull measurements have been included in order to evaluate the performance of the amplifiers operating with variable source impedances. Noise temperatures below 55 K have been obtained for the differential design in the 300–1000-MHz band for the 150-$Omega$ impedance. In addition, the results for different scanning angles are also presented.
机译:本文将差分低噪声放大器作为射电天文应用的一种非常强大的解决方案。全微分放大器拓扑已通过微带技术进行了分析,并采用了分立的表面安装元件。该放大器设计用于有源接收密集天线阵列。因此,差分放大器的源阻抗不再是50ΩΩ,而是150ΩΩ。已经进行了增益和噪声方面的全面表征。为了评估在可变源阻抗下工作的放大器的性能,已经包括了源-挽测量。对于150-Ω阻抗,在300-1000MHz频段内进行差分设计时,已获得低于55 K的噪声温度。此外,还介绍了不同扫描角度的结果。

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