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Tunable Narrow-Band Filter for Imaging Polarimetry

机译:用于成像偏振器的可调窄带滤波器

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A fully tunable narrow-band filter system to be used in combination with ZIMPOL for monochromatic imaging vector polarimetry is being developed. It may be used over the whole visible spectrum, from the t.JV at about 395 nm, to the red at about 660 nm, with a band width of 30-50 rnA. The main components are two lithium-niobate Fabry-Perot etalons made of Y-cut crystals, which means that the channel spectra and tuning parameters are different for the two orthogonal states of polarization (ordinary and extraordinary rays). This allows the finesse to be dramatically enhanced by a double-pass configuration, a possibility that is not available to other Fabry-Perot systems. Tuning can be achieved in three ways: temperature tuning to center the pass band within the selected fine tuning range, voltage tuning for rapid fine tuning, and tilt tuning as an additional, though normally not used, possibility. The filter system will allow us to explore the spatial structuring of the polarization signatures in the Second Solar Spectrum, including vector mapping of the Hanle and Zeeman effects in any spectral line between the UV and red part of the spectrum.
机译:正在开发一个完全可调窄带滤波器系统,用于组合用于单色成像矢量偏振物的ZIMPOL。它可以在整个可见光谱中,从T.JV在约395nm处,在约660nm的红色,带宽度为30-50 rna。主要成分是由Y切割晶体制成的两个锂 - 铌酸锂法布里 - 珀罗·珀罗龙,这意味着对极化(普通和非凡射线)的两个正交状态不同的通道谱和调谐参数是不同的。这允许通过双通配置大大提高了技巧,其它法布里 - 珀罗系统不可用的可能性。调整可以通过三种方式实现:温度调谐到中心的通频带内所选择的微调范围,电压调谐用于快速微调,以及倾斜调谐,虽然通常不使用,但可能性。过滤系统将允许我们探讨第二太阳频谱中的偏振签名的空间结构,包括在频谱的UV和红色部分之间的任何光谱线中的Hanle和Zeeman效果的矢量图。

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