接收信号初步处理阶段的射频干扰抑制方法

Q4 Physics and Astronomy Radio Physics and Radio Astronomy Pub Date : 2022-01-01 DOI:10.15407/rpra27.04.268
L. Stanislavsky
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引用次数: 1

摘要

主题和目的。给出了空间天体低频射电天文信号的计算机处理方法。本文的目的是改进现有的方法,并利用它们的组合在频域上清除自然和人工来源的无线电干扰,并讨论这些方法的优缺点。方法和方法论。在对射电天文观测记录的研究中,有一个共同的特点,即从空间源接收到的信号都有无线电干扰的显著贡献。在对可能的干扰类型和信号在其传播方式上的失真有足够的经验后,所建议的程序的效率被显示出来,通过不同方法的组合,根据所调查空间物体信号的典型特征,在频率-时间域清除无线电信号干扰。结果。在干扰背景下提取空间信号的发展方法使人们能够获得天体物理现象中射电发射源的独特数据。一方面,软件工具可以在无线电频率干扰的背景下检测到非常微弱的事件。另一方面,它们允许人们根据统计上最完整的事件集来测量发射参数。结论。这项工作的结果表明,由于射电干扰,没有普遍的方法来克服射电天文观测记录中的任何障碍。此外,即使采用了最适当的方法,也往往需要预先调整相应的参数,而对产生区域的无线电发射的物理参数的分析则依赖于这些参数。但是,如果这样的空间信号在无线电记录中没有被干扰严重破坏,那么使用经过考虑的方法可能是成功和有用的。
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METHODS OF RADIO FREQUENCY INTERFERENCE MITIGATION ON THE STAGE OF PRELIMINARY PROCESSING OF RECEIVED SIGNALS
Subject and Purpose.Methods for computer processing of radio astronomical signals observed with space objects at low frequencies are given. The aim of this paper is to improve the current methods and use their combinations for cleaning records from radio interference of natural and artificial origin in the frequency-time domain, as well as to discuss advantages and disadvantage of the methods. Methods and Methodology.In the study of records obtained with radio astronomical observations there is a common feature of received signals from space sources, which consists in a significant contribution of radio interference. Having sufficient experience on possible types of interference and distortion of signals on the way of their propagation, the efficiency of suggested procedures, clearing radio signal interference in the frequency-time domain by a combination of different approaches in dependence from typical features of signals withinvestigated space objects, is shown. Results. The developed methods of extracting space signals against the background of interference allow one to get unique data on the sources of radio emission in astrophysical phenomena. On the one hand, software tools make it possible to detect very weak events against the background of radio frequency interference. On the other hand, they allow one to measureemission parameters based on the most statistically complete set of events. Conclusions.The results obtained in this work manifest that there is no universal way to overcome any obstacle in the records of radio astronomical observations because of radio interference. In addition, even if the most appropriate method is applied, it often requires pre-adjustment of the corresponding parameters on which the analysis of physical parameters of radio emission in the area of generation depends. But if such a space signal at the radio records is not very spoiled by interference, the use of considered methods can be successful and useful.
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来源期刊
Radio Physics and Radio Astronomy
Radio Physics and Radio Astronomy Physics and Astronomy-Physics and Astronomy (miscellaneous)
CiteScore
0.60
自引率
0.00%
发文量
18
审稿时长
8 weeks
期刊最新文献
GROUND BASED SUPPORT OF THE SPACE MISSION PARKER PERFORMED WITH UKRAINIAN LOW FREQUENCY RADIO TELESCOPES FRACTAL RADIOPHYSICS. Part 2. FRACTAL AND MULTIFRACTAL ANALYSIS METHODS OF SIGNALS AND PROCESSES OMNIDIRECTIONAL MILLIMETER-WAVELENGTH ANTENNAS BASED ON SEGMENTAL DIELECTRIC RESONATORS WHICH SUPPORT WHISPERING GALLERY MODES V. P. SHESTOPALOV AND HIS SCIENTIFIC SCHOOL: FROM QUASISTATICS TO QUASIOPTICS (to mark V.P.'s birth centenary) PROGRESS IN THE STUDY OF DECAMETER-WAVELENGTH SOLAR RADIO EMISSION WITH UKRAINIAN RADIO TELESCOPES. Part 1. (Invited paper)
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