A High Time Resolution Polarimeter Spectrometer for Radio Astronomy

P. J. Hall
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Abstract

This paper describes a high time resolution radio polarimeter spectrometer based on SAW spectrum analysers. The bandwidth of the prototype instrument is about 30 Xz; time and frequency resolutions of the basic processor are 2.4 us and 650 kHz. Spectra for the Stokes wave polarization parameters are obtainable, allowing complete characterization of incident radiation. The data rate problem usually encountered when SAW chirp Fourier transformers are interfaced to digital post-transformation processors has been overcome with the development of a fast, digital spectrum integrator. This allows the SAW IF processor to work in conjunction with general-purpose computers, giving an observing system with an overall time resolution of around 150 ps. The radiometric efficiency of the new instrumentation compares favourably with that of other radio astronomy spectrometers.
用于射电天文学的高时间分辨率偏振计光谱仪
介绍了一种基于声表面波频谱分析仪的高时间分辨率无线电偏振计光谱仪。样机的带宽约为30xz;基本处理器的时间和频率分辨率分别为2.4 us和650 kHz。光谱的斯托克斯波极化参数是可获得的,允许入射辐射的完整表征。随着快速数字频谱积分器的发展,SAW啁啾傅立叶变压器与数字后变换处理器接口时经常遇到的数据速率问题已经得到了克服。这允许SAW中频处理器与通用计算机一起工作,提供一个整体时间分辨率约为150 ps的观测系统。新仪器的辐射测量效率与其他射电天文光谱仪相比是有利的。
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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