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East-West Fourier Transforms of Polarization Parameters of Radio Sources at 1418 MHz

机译:1418 MHz无线电源极化参数的东西向傅里叶变换

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摘要

As part of a continuing study employing the Owens Valley Radio Observatory's twin-element interferometer to provide high angular resolution measurements of the various radio source properties (see, especially, Maltby and Moffett 1962; Morris, Radhakrishnan, and Seielstad 1964b; Seielstad 1967; Fomalont 1968), we have measured the Fourier transforms of the distributions of the Stokes parameters Q, U, and V at several antenna spacings along an east-west baseline. The present paper catalogs these measurements, while a subsequent paper will interpret them in terms of the structure of the polarized radiation along a circle of constant declination. We have already published a list of upper limits to the degree of circular polarization in the integrated radiation from several of these sources (Seielstad and Weiler 1968a), as well as a complete analysis of four supernova remnants (Seielstad and Weiler 1968b).
机译:作为一项持续研究的一部分,该研究利用欧文斯谷射电天文台的双元件干涉仪提供了各种无线电源特性的高角分辨率测量(尤其是参见Maltby和Moffett 1962; Morris,Radhakrishnan和Seielstad 1964b; Seielstad 1967; Fomalont 1968年),我们已经测量了沿东西向基线在几个天线间距处斯托克斯参数Q,U和V的分布的傅立叶变换。本文对这些测量进行了分类,而随后的论文将根据沿恒定磁偏角圆的偏振辐射的结构来解释它们。我们已经发布了来自这些来源中的几个的积分辐射中圆极化程度的上限列表(Seielstad和Weiler 1968a),以及对四个超新星残骸的完整分析(Seielstad和Weiler 1968b)。

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