大气探测和射电天文学用毫米波和亚毫米波外差接收机

G. Beaudin, A. Deschamps, P. Encrenaz, P. Feautrier, P. Febvre, M. Gheudin, O. Perrin, J. Pernot, C. Prigent, C. Robert, G. Ruffle
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引用次数: 1

摘要

为了准备气象和天体物理学的空间计划,法国航天局(CNES)支持开发了两种外差仪器:用于大气探测的十通道毫米波辐射计;和一个气球载天文台(PRONAOS),包括一个2米望远镜和一个用于射电天文学的亚毫米外差光谱仪。该接收机包括一个工作在4k的Nb/AlO/sub x//Nb隧道结的SIS混频器,一个6 GHz中频低噪声冷却前置放大器,一个LO准光注入锁相Gunn振荡器和两个级联倍频器。噪声温度低至300 K;预计少于20万。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Millimetre And Submillimetre Wave Heterodyne Receivers For Atmospheric Sounding And Radioastronomy
To prepare the space programs on meteorology and astrophysics, the development of two heterodyne instruments has been supported by the French Space Agency (CNES): a ten channels millimetre wave radiometer for atmospheric sounding; and a balloon-borne observatory (PRONAOS) including a 2 metre telescope associated with a submillimetre heterodyne spectrometer for radioastronomy. This receiver includes a SIS mixer using Nb/AlO/sub x//Nb tunnel junctions operating at 4 K, a 6 GHz IF low-noise cooled preamplifier, a LO quasi-optically injected with a phase locked Gunn oscillator and two cascaded frequency multipliers. Noise temperature as low as 300 K has been obtained; less than 200 K is expected.
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