射电天文学中信号处理算法验证的相干信号生成

T. Gunaratne
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引用次数: 2

摘要

下一代射电望远镜(如SKA, ngVLA)需要满足严格的信号质量要求。仿真方法已广泛应用于这些望远镜信号链的设计和验证。模拟方法的一个关键方面是产生相干的“类噪声”测试序列,模拟天体辐射和由于地球自转而导致的不同受体的传播延迟变化。这些射电望远镜信号链的大抽取因子要求产生长序列的相干宽带信号。本文提出了一种基于chirp-z变换(CZT)产生宽带相干伪随机测试序列的有效方法。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Generation of Coherent Signals for the Verification of Signal Processing Algorithms in Radio Astronomy
Next generation radio telescopes (e.g. SKA, ngVLA) are required to meet stringent requirements in signal quality. Simulation methods have been extensively used for both design and verification of the signal chains of these telescopes. A key aspect of the simulation methods is the generation of coherent ‘noise-like’ test sequences that mimic celestial radiation and the variation of propagation delays to the different receptors due to the rotation of the Earth. The large decimation factors associated with the signal chains of these radio telescopes require the generation of long sequences of coherent wideband signals. An efficient method based on the chirp-z transform (CZT) for generating wideband coherent pseudo-random test sequences is presented in the following.
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