首页> 外文会议>International SYmposium on Temperature and Thermal Measurements in Industry and Science >A MONTE CARLO CALCULATION OF LENS ABBERATION EFFECT ON THE SIZE OF SOURCE EFFECT IN RADIATION PYROMETRY
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A MONTE CARLO CALCULATION OF LENS ABBERATION EFFECT ON THE SIZE OF SOURCE EFFECT IN RADIATION PYROMETRY

机译:辐射高温计源效应尺寸的蒙特卡罗计算

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The size of source effect (SSE) is one of the most serious components of uncertainty sources in the primary pyrometry and the radiometry. The SSE is originated from aberration, diffraction, and scattering. To optimize design of pyrometers and improve the uncertainty of the temperature scales, a calculation of the aberration effect on the SSE is necessary. We have calculated effect of objective lens aberrations on the SSE by the Monte Carlo method. The source was assumed uniform and Lambertian. Random numbers determined positions on the source rays emerged from and the direction the rays traveled. Trajectories of rays were calculated by the ray tracing until the ray struck a screen after passing through the lens. The number of rays that struck each annulus predefined on the screen was counted to give an amplitude distribution of radiance level on the image plane. The distributions were calculated as increasing the dimension of the source to yield the SSE. The defocus effect of the SSE was also calculated by changing the screen distance from the best focus. The results were discussed with comparison to measurement of the KRISS standard pyrometer of which the minimum target size is 0.8 mm in diameter. Aberrations of the objective lens in the KRSS pyrometer gave the most critical effect to SSE in the range where the source size is less than 2 times of the minimum target size in diameter.
机译:源效应(SSE)的大小是初级热测定和辐射测定中的不确定源最严重的组件之一。 SSE起源于像差,衍射和散射。为了优化高温计的设计,提高温度尺度的不确定性,需要对SSE进行像差效应的计算。我们通过Monte Carlo方法计算了物镜像差对SSE上的物镜差的影响。源是假设统一和兰伯特的。随机数确定源光线上的位置,并且射线行进的方向。通过光线跟踪计算光线的轨迹,直到通过镜头后射线击中屏幕。计数在屏幕上撞击预定义的每个环空的光线的数量,以在图像平面上产生辐射电平的幅度分布。分布计算为增加源的尺寸以产生SSE。还通过从最佳焦点改变屏幕距离来计算SSE的散焦效果。与测量的Kriss标准高温计的测量相比,讨论了该结果,其中最小目标尺寸为0.8mm。 KRSSS的物镜的像差在源尺寸小于直径最小目标尺寸的2倍的范围内对SSE产生最关键的效果。

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