首页> 外文会议>American Radio Relay League,Inc.(ARRL) and Tucson Amateur Packet Radio(TAPR) Digital Communications Conference; 20040910-12; Des Moines,IA(US) >DESIGN AND IMPLEMENTATION OF RECEIVER SYSTEM FOR SUPPPRESSING RADIO FREQUENCY INTERFERENCE USING ADAPTIVE FILTERS
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DESIGN AND IMPLEMENTATION OF RECEIVER SYSTEM FOR SUPPPRESSING RADIO FREQUENCY INTERFERENCE USING ADAPTIVE FILTERS

机译:自适应滤波器抑制无线电频率干扰的接收机系统的设计与实现

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Radio Frequency Interference (RFI) is increasingly affecting radio astronomy observations. Recent interference mitigation techniques developed for communication engineering have been applied in radio astronomy. However, RFI rejection achieved till now is not sufficient for radio astronomy. Research in developing new techniques is therefore essential. This paper describes an improvised technique of RFI suppression by adaptive filters by constraining the bandwidth of the reference signal and also to study the effects of quantisation of bits to suppress RFI. The adaptive cancellation technique requires two receivers: a primary channel that will be the radio telescope and a reference channel. For this experimental research, a reference receiver system has been designed and built which could be used along with the existing 10.4m diameter radio telescope functioning at Raman Research Institute, Bangalore. The receiver setup is designed around the 1.4 GHz receiver system of the 10.4-m telescope, and thus the research is to mitigate RFI in the 1.4204 GHz frequency band. The reference antenna system constructed is used to receive the man made RFI .The bandwidth of the reference signal is reduced by 25 MHz and then is processed by an adaptive filter .The 1.4 GHz signal from the telescope and antenna are down converted to 50MHz and connected to a data recording system. By simulations in Matlab, we studied the effect of constraining the bandwidth of reference signal on the suppression achieved in a LMS adaptive filter when the signal to noise ratio of the RFI in the reference channel is moderate. It is found that constraining the bandwidth.
机译:射频干扰(RFI)越来越多地影响射电天文观测。为通信工程开发的最新干扰缓解技术已应用于射电天文学。但是,到目前为止,射频干扰的拒绝还不足以解决射电天文学。因此,研究开发新技术至关重要。本文通过限制参考信号的带宽,描述了一种通过自适应滤波器抑制RFI的改进技术,并研究了比特量化对抑制RFI的影响。自适应抵消技术需要两个接收器:一个将成为射电望远镜的主信道和一个参考信道。为了进行这项实验研究,已经设计并制造了一个参考接收器系统,该系统可以与班加罗尔拉曼研究所的现有直径为10.4m的射电望远镜一起使用。接收器设置是围绕10.4 m望远镜的1.4 GHz接收器系统设计的,因此研究旨在减轻1.4204 GHz频带中的RFI。所构建的参考天线系统用于接收人造RFI。参考信号的带宽减少25 MHz,然后由自适应滤波器处理。来自望远镜和天线的1.4 GHz信号下变频为50MHz并连接到数据记录系统。通过在Matlab中进行仿真,我们研究了在参考通道中RFI的信噪比适中时,限制参考信号带宽对LMS自适应滤波器实现的抑制效果。发现限制了带宽。

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