Deep, Broad Null Formation for Canceling Moving RFI in Radio Astronomical Arrays

IF 1.5 Q3 ASTRONOMY & ASTROPHYSICS
R. Black, B. Jeffs, K. Warnick
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引用次数: 1

Abstract

Radio frequency interference (RFI) is rapidly becoming a major issue for many applications. It is especially problematic for radio astronomy, where signal-to-noise ratios (SNRs) are less than unity. Antenna array systems such as phased array feeds (PAFs) and interferometric imaging arrays are able to cancel RFI through adaptive projection-based spatial notch filtering techniques. Current methods for formulating these projection operators suffer from an unfortunate trade-off. They must sacrifice integration time when calculating the sample spatial correlation matrix in order to track RFI motion, but this consequently increases sample estimation error and reduces null depth. In this work, we propose a new way to process spatial correlation matrices to form a broad null that reliably cancels moving RFI without increasing sample estimation error due to insufficient integration. Additionally, when assisted by an RFI-tracking auxiliary antenna, this approach also reduces the total data rate coming out of a spatial correlator, thus making broad-null-based RFI cancelation more computationally efficient and practical for real-time active array-based RFI mitigation systems.
用于消除射电天文阵列中移动射频信号的深宽零阵
射频干扰(RFI)正迅速成为许多应用的主要问题。这对射电天文学来说尤其有问题,因为那里的信噪比(SNR)小于一。诸如相控阵馈电(PAF)和干涉成像阵列之类的天线阵列系统能够通过基于自适应投影的空间陷波滤波技术来消除RFI。目前制定这些投影算子的方法遭遇了不幸的权衡。当计算样本空间相关矩阵以跟踪RFI运动时,它们必须牺牲积分时间,但这会增加样本估计误差并减少零深度。在这项工作中,我们提出了一种新的方法来处理空间相关矩阵,以形成一个广泛的零点,该零点可靠地消除了移动RFI,而不会因积分不足而增加样本估计误差。此外,在RFI跟踪辅助天线的辅助下,这种方法还降低了来自空间相关器的总数据速率,从而使基于零的广义RFI消除在计算上更高效,对于基于实时有源阵列的RFI缓解系统更实用。
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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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