Multi-frequency SuperDARN interferometer calibration

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2024-07-01 DOI:10.1029/2024RS007957
E. G. Thomas;S. G. Shepherd;G. Chisham
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引用次数: 0

Abstract

The ground-based, high-frequency radars of the Super Dual Auroral Radar Network (SuperDARN) observe backscatter from ionospheric field-aligned plasma irregularities and features on the Earth's surface out to ranges of several thousand kilometers via over-the-horizon propagation of transmitted radio waves. Interferometric techniques can be applied to the received signals at the primary and secondary antenna arrays to measure the vertical angle of arrival, or elevation angle, for more accurate geolocation of SuperDARN observations. However, the calibration of SuperDARN interferometer measurements remains challenging for several reasons, including a 2π phase ambiguity when solving for the time delay correction factor needed to account for differences in the electrical path lengths between signals received at the two antenna arrays. We present a new technique using multi-frequency ionospheric and ground backscatter observations for the calibration of SuperDARN interferometer data, and demonstrate its application to both historical and recent data.
多频超级雷达网干涉仪校准
超级双极光雷达网(SuperDARN)的地基高频雷达通过发射无线电波的超视距传播,观测电离层场对齐等离子体的反向散射和地球表面的特征,其范围可达数千公里。干涉测量技术可应用于主天线阵列和副天线阵列接收的信号,以测量垂直到达角或仰角,从而更准确地确定超级雷达网观测的地理位置。然而,超级雷达网干涉仪测量的校准工作仍具有挑战性,原因有几个,其中包括在求解时间延迟校正因子时存在 2π 的相位模糊性,而时间延迟校正因子需要考虑两个天线阵列接收信号的电路径长度差异。我们提出了一种利用多频电离层和地面反向散射观测来校准超级雷达网干涉仪数据的新技术,并演示了该技术在历史数据和最新数据中的应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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