人口密度对选定CALLISTO台站动态频谱射频干扰(RFI)分析的影响研究

Z. N. Zainud-din, N. Sabri, Roslan Umar, C. Monstein
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摘要

射频干扰(RFI)是近年来射电天文观测中的一个重要问题。紧凑型低成本天文光谱学可移动天文台仪器(CALLISTO)是一个用于太阳活动监测的全球性光谱仪系统网络。由于射频干扰,对太阳射电爆发的探测被中断,因为这些电台都设在地面上。由于RFI信号是从周围检测到的,这为地面基站的观测提供了不准确的数据。rfisource主要来自人造设备。本文采用峰度分析方法对选定callistostation的RFI水平进行了分析。来自马来西亚万廷、印尼苏梅当、印度印度和韩国大田的两个月(45-870 MHz)的数据被选中,这些数据包含太阳爆发和没有太阳爆发。然后将峰度值与种群密度进行比较,得到种群密度与RFI水平之间的关系。峰度值的最高平均值表示这些位置的射频干扰最低。使用MATLAB软件进行数据分析,使用microsoft Excel进行RFI分析绘图。结果表明,高人口密度并不是造成周边干扰的主要因素。关键词:射频干扰,射电天文学,峰度分析,e-CALLISTO
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The study on the effect of population density on radio frequency interference (RFI) analysis on dynamic spectrum at selected CALLISTO stations
Radio Frequency Interference (RFI) has become a critical issue in radio astronomy observation in recentyears. Compact Astronomical Low-Cost Instrument for Spectroscopy in Transportable Observatories(CALLISTO) is a worldwide network of spectrometer system for solar activity monitoring. The detection ofsolar radio bursts is being interrupted due to RFI as these stations are held on the ground. Since RFI signalsare being detected from surrounding, this gives inaccurate data for ground base station observations. RFIsources are mostly from man-made devices. This paper study analysis of RFI level at selected CALLISTOstations by using Kurtosis Analysis. Data from Banting, Malaysia, Sumedang, Indonesia, Ooty, India andDaejeon, South Korea stations for two months (45–870 MHz) that contain solar burst and no solar bursthad been selected. The kurtosis value is then compared with the population density to get the relationshipbetween the population density and the RFI level. The highest average of kurtosis value indicates thelowest of radio frequency interference at these sites. MATLAB software was used for the data analysis andMicrosoft Excel for the RFI profiling graphing. The results show that the high population density is not amain factor that contributes the interference towards the surrounding. Key words: Radio Frequency Interference (RFI), radio astronomy, kurtosis analysis, e-CALLISTO.
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