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Measurement of polarization assemblies for the Daniel K. Inouye Solar Telescope

机译:Daniel K. Inouye太阳望远镜的偏振组件的测量

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We present here methodology and instrumentation for the precise measurement of retardance and optic axis orientation of retarder assemblies for the Daniel K. Inouye Solar Telescope. This solar telescope will perform broadband polarimetry of the sun. Each Meadowlark assembly is made up of three compound zero order retarders that must have a retardance variation of less than 6.33 nanometers across the greater than 110 millimeter clear aperture. The retardation of each component was measured using a combination of spectral transmission scans and ellipsometry, with test wavelengths of less than a 0.45 nanometer bandwidths and yielding a standard deviation in measurements of less than 0.001 waves. A technique for the measurement of the near zero window (Infrasil® and CaF_2) retardance is shown, in addition to retardance measurements of the component waveplates. An average retardance of 0.63 ran for CaF_2 and 0.28 ran for Infrasil® was found. Finally, a technique for determining the optic axis tilt of each crystal waveplate using laser ellipsometry is discussed.
机译:我们在此介绍用于Daniel K.Inouye太阳望远镜的延迟器组件的延迟和光轴方向的精确测量的方法和仪器。该太阳望远镜将对太阳进行宽带极化分析。每个Meadowlark组件均由三个复合零级延迟器组成,这些延迟器必须在大于110毫米的透明孔径上具有小于6.33纳米的延迟变化。使用光谱透射扫描和椭圆偏振法的组合来测量每种组分的延迟,其测试波长小于0.45纳米带宽,并且在测量中产生的标准偏差小于0.001波。除了分量波片的延迟测量之外,还显示了一种用于测量接近零窗口的延迟(Infrasil®和CaF_2)的技术。发现CaF_2的平均延迟为0.63 ran,Infrasil®的平均延迟为0.28 ran。最后,讨论了使用激光椭圆偏振法确定每个晶体波片的光轴倾斜的技术。

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