首页> 外文期刊>International Journal of Astronomy and Astrophysics >Creating a “Faraday Ghost” inside the Rotation Measure Synthesis Technique, through a Wide Observational “Gap” in Wavelength Coverage
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Creating a “Faraday Ghost” inside the Rotation Measure Synthesis Technique, through a Wide Observational “Gap” in Wavelength Coverage

机译:通过在波长覆盖范围内观察到较大的“间隙”,在旋转量度合成技术中创建“法拉第重影”

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Several recently published Faraday rotation measures (RM) derived using the novel RM synthesis technique are likely in error. If a set of polarimetric observations contains a large gap in the wavelength coverage, the rotation measure determination is sometimes ambiguous; this is also true even when two long wavelength ranges are observed but are separated by a wide gap. Essentially, there are 180° ambiguities in the observed Position Angle of the electric polarisation vector between the two wavelength ranges; these ambiguities are not resolved because the extent of wavelengths2 covered, within each of the two ranges, is too small to uniquely determine the RM in isolation. We find that unphysical “Faraday ghosts” can be mathematically constructed with a np ambiguity (±180° times an integer) at predictable polarization position angles when using only two wavelength ranges separated by a gap, as a function of the width of the gap (Equation (4)). Our computations suggest an empirical correlation between an observational gap between two wavelength ranges and the appearance of “Faraday ghosts”.
机译:使用新的RM合成技术得出的一些最近发布的法拉第旋转量度(RM)可能有误。如果一组极化观测结果在波长范围内包含较大的间隙,则旋转量度的确定有时会模棱两可;即使观察到两个很长的波长范围,但它们之间的间隔很大,这也是正确的。本质上,在两个波长范围之间观察到的极化矢量的位置角存在180°的歧义。这些不确定性无法解决,因为在两个范围的每个范围内所覆盖的波长范围太小,无法单独确定RM。我们发现,当仅使用两个由间隙隔开的波长范围时,可以通过可预测的偏振位置角度以np歧义(±180°乘以整数)在数学上构造非物理的“法拉第鬼影”,该函数是间隙的宽度(等式(4))。我们的计算表明两个波长范围之间的观察间隙与“法拉第重影”的出现之间存在经验相关性。

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