Radioastron 22ghz接收机的空间鉴定

P. Piironen, J. Mallat, A. Rasanen, E. Siivola, J. Takala, P. Jukkala, P. Sailamaki, H. Somerma, J. Ylinen
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引用次数: 3

摘要

预计将于1995年发射的Radioastron空间VLBI卫星将载有四个灵敏的双通道辐射计。芬兰负责22ghz的接收器。接收机最重要的性能是灵敏度、相位稳定性和增益稳定性。为了达到最大的灵敏度,设计了一种符合现代空间要求的低噪声HEMT放大器。测得的接收机噪声温度为140k。为了获得最大相位和振幅稳定性,采用了温度稳定和高Q介电谐振振荡器设计。所测相稳定性优于3 0 /h。介绍了空间定性试验和可靠性分析的主要内容。
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Space Qualification of the Radioastron 22 GHz Receiver
The Radioastron space VLBI satellite, expected to be launched in 1995, will have on board four sensitive two-channel radiometers. Finland is responsible for the 22 GHz receiver. The most important properties of the receiver are sensitivity, phase stability and gain stability. To reach maximum sensitivity, a modern space qualified low noise HEMT amplifier has been designed. The measured receiver noise temperature is 140 K. For maximum phase and amplitude stabilities, temperature stabilisation and a high Q dielectric resonator oscillator design have been utilized. The measured phase stability is better than 3 o/h. The main aspects of the space qualification tests and the reliability analysis are described.
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