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System Temperature Characterization of Nkutunse Receiver at 5GHz (Continuum) and 6.7GHz (Methanol Maser)

机译:Nkutunse接收器在5GHz(Continuum)和6.7GHz(甲醇Maser)上的系统温度特性

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This paper presents the characterization of system temperature (Tsys) for the first stage receiver of the 32 m diameter cassegrain antenna at Nkutunse (Ghana) with a hot load jig. The hot load jig was place above the Beam Wave Guide and the Feed horn and the noise diode switched ON and OFF. The recorded Tsys values at 5 GHz (Continuum) was 160 K and at 6.7 GHz (Methanol Maser) was 120 K. These high Tsys values, is as a result of using one LNA in the first stage. The conducted measurement considered both right hand cross polarization (RHCP) and left hand cross polarization (LHCP) of the signal chain. With cascaded LNAs in the final stage of the receiver, it is certain the required 75 K for the telescope operation can be achieved. However, a second approach to keep the Tsys in check means that Radio Frequency Interference (RFI) at the site should be mitigated, since it adds to the cumulative noise power of a system and thereby reducing the sensitivity of the receiver.
机译:本文介绍了Nkutunse(加纳)带有热负载夹具的直径为32 m的c形天线第一级接收器的系统温度(Tsys)的特性。将热负载夹具放在光束波导和馈电喇叭上方,并且将噪声二极管打开和关闭。在5 GHz(连续谱)下记录的Tsys值为160 K,在6.7 GHz(甲醇Maser)下记录的Tsys值为120K。这些高Tsys值是在第一阶段使用一个LNA的结果。进行的测量同时考虑了信号链的右手交叉极化(RHCP)和左手交叉极化(LHCP)。在接收器的最后阶段使用级联LNA,可以确定望远镜操作所需的75K。但是,第二种控制Tsys的方法意味着应减轻现场的射频干扰(RFI),因为它会增加系统的累积噪声功率,从而降低接收器的灵敏度。

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