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

机译:达尼尔K. inouye太阳能望远镜的偏振组件测量

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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:我们在这里介绍了Daniel K. Inouye太阳能望远镜延迟器组件的延迟和光学轴取向的精确测量方法和仪表。这张太阳望远镜将执行太阳的宽带偏振基。每个Meadowlark组件由三个复合零级延迟器组成,其必须在大于110毫米透明孔径上具有小于6.33纳米的延迟变化。使用光谱传输扫描和椭圆形测量的组合测量每个组分的延迟,测试波长小于0.45纳米带宽,并在测量值小于0.001波的测量中产生标准偏差。除了组件波形的延迟测量之外,还示出了用于测量近零窗口(Infasilα和CAF_2)延迟的技术。对于CAF_2和0.28 ran用于i​​nfasil的平均延迟为0.63 ran?被找到。最后,讨论了一种用于使用激光椭圆形测定的每个晶体波片的光轴倾斜的技术。

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