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Phase-disturbing speckle-suppressing method in fiber metrology under coherent illumination

机译:相干照明下光纤计量中的干扰相干斑点抑制方法

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When we use laser to measure the focal ratio degradation of astronomical fibers, we have to reduce the speckle contrast to fit the output spot to a 2-D Gaussian-like function. The origin speckle contrast is near to 100%. The simple average method doesn't work because the speckle patterns are stable. We tried several ways to disturb randomly the transmission phase of the light modes inside the fiber to be tested. Both non-contact fiber-disturb-mode device (NCFDMD) and contact fiber-disturb-mode device (CFDMD) were established and tested. The NCFDMD is to set a vibrating phase plate against the output end of the tested fiber. The CFDMD is to set the vibrating device in the middle of the fiber. Under different vibration frequency we compared the contrast of speckle patterns. We set different exposure time of the CCD camera to check the effects. For NCFDMD, the exposure time should be long enough, for example 30 ms, to guarantee enough different patterns could be collected to suppress the contrast of the speckle and get good Gauss-like pattern. For CFDMD, we compared three kinds of fibers with different core-diameters. We found that 65-70 Hz is the optimized vibration frequency for all fibers and 30 ms is the best exposure time. The introduction of the phase modulation could dramatically suppress the speckle under coherent illumination. The measurement accuracy could be enhanced according to the speckle suppression.
机译:当我们使用激光测量天文纤维的焦比降低时,我们必须降低斑点对比度,以使输出光斑适合二维高斯函数。原点斑点对比度接近100%。简单的平均方法不起作用,因为斑点图案稳定。我们尝试了几种方法来随机干扰要测试的光纤内部的光模式的传输阶段。建立并测试了非接触式光纤干扰模式设备(NCFDMD)和接触式光纤干扰模式设备(CFDMD)。 NCFDMD将振动相板置于被测光纤的输出端。 CFDMD用于将振动装置设置在光纤中间。在不同的振动频率下,我们比较了斑点图案的对比度。我们设置了CCD相机的不同曝光时间以检查效果。对于NCFDMD,曝光时间应足够长,例如30 ms,以确保可以收集到足够多的不同图案以抑制斑点的对比度并获得良好的高斯状图案。对于CFDMD,我们比较了三种具有不同纤芯直径的光纤。我们发现65-70 Hz是所有光纤的最佳振动频率,而30 ms是最佳的曝光时间。相位调制的引入可以极大地抑制相干照明下的斑点。根据斑点抑制,可以提高测量精度。

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