Performance Analysis Techniques for Real-time Broadband RFI Filtering System of uGMRT

IF 1.5 Q3 ASTRONOMY & ASTROPHYSICS Journal of Astronomical Instrumentation Pub Date : 2022-03-01 DOI:10.1142/S2251171722500088
K. Buch, R. Kale, K. Naik, Rahul Aragade, M. Muley, S. Kudale, Ajith Kumar
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引用次数: 1

Abstract

Electromagnetic radiation from human activities, known as man-made Radio Frequency Interference (RFI), adversely affects radio astronomy observations. In the vicinity of the Upgraded Giant Metrewave Radio Telescope (uGMRT) array, the sparking on power lines is the major cause of interference at observing frequencies less than 800 MHz. A real-time broadband RFI detection and filtering system is implemented as part of the uGMRT wideband signal processing backend to mitigate the effect of broadband RFI. Performance analysis techniques used for testing and commissioning the system for observations in the beamformer and correlator modes of the uGMRT are presented. The concept and implementation of recording simultaneous unfiltered and filtered data along with data analysis and interpretation is illustrated using an example. For the beamformer mode, spectrogram, single spectral channel, and its Fourier transform is used for performance analysis whereas, in the correlator mode, the cross-correlation function, closure phase, and visibilities from the simultaneously recorded unfiltered and filtered is carried out. These techniques are used for testing the performance of the broadband RFI filter and releasing it for uGMRT users.
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uGMRT实时宽带RFI滤波系统性能分析技术
人类活动产生的电磁辐射,即人造射频干扰,对射电天文学观测产生不利影响。在升级后的巨型米波射电望远镜(uGMRT)阵列附近,电源线上的火花是观测频率低于800 MHz时干扰的主要原因。作为uGMRT宽带信号处理后端的一部分,实现了实时宽带RFI检测和滤波系统,以减轻宽带RFI的影响。介绍了用于测试和调试uGMRT波束形成器和相关器模式下观测系统的性能分析技术。通过一个例子说明了同时记录未过滤和过滤数据以及数据分析和解释的概念和实现。对于波束形成器模式,频谱图、单频谱通道及其傅立叶变换用于性能分析,而在相关器模式中,执行来自同时记录的未滤波和滤波的互相关函数、闭合相位和可见性。这些技术用于测试宽带RFI滤波器的性能,并将其发布给uGMRT用户。
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来源期刊
Journal of Astronomical Instrumentation
Journal of Astronomical Instrumentation ASTRONOMY & ASTROPHYSICS-
CiteScore
2.30
自引率
7.70%
发文量
19
期刊介绍: The Journal of Astronomical Instrumentation (JAI) publishes papers describing instruments and components being proposed, developed, under construction and in use. JAI also publishes papers that describe facility operations, lessons learned in design, construction, and operation, algorithms and their implementations, and techniques, including calibration, that are fundamental elements of instrumentation. The journal focuses on astronomical instrumentation topics in all wavebands (Radio to Gamma-Ray) and includes the disciplines of Heliophysics, Space Weather, Lunar and Planetary Science, Exoplanet Exploration, and Astroparticle Observation (cosmic rays, cosmic neutrinos, etc.). Concepts, designs, components, algorithms, integrated systems, operations, data archiving techniques and lessons learned applicable but not limited to the following platforms are pertinent to this journal. Example topics are listed below each platform, and it is recognized that many of these topics are relevant to multiple platforms. Relevant platforms include: Ground-based observatories[...] Stratospheric aircraft[...] Balloons and suborbital rockets[...] Space-based observatories and systems[...] Landers and rovers, and other planetary-based instrument concepts[...]
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