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Calibration on the Spectral Radiance of Integral Sphere

机译:积分球光谱辐射率的校准

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We have to make the integral sphere source trace to the standard lamp, when we calibrate the imaging spectrometer. But the standard lamp need to be calibrated by the blackbody firstly. In this paper, we have the integral sphere source trace to the blackbody directly, using the exclusive spectral response of a spectrometer. During the experiments, two spectral responses of thernspectrometer (200nm ~ 1100nm) within 700nm ~ 900nm are obtained separately by measuring thernspectral radiances of the blackbody at 1000℃ and the integral sphere source at some colorrntemperature. We get the equivalent color temperature of the integral sphere source, making use of the consistency of the two spectral responses in theory. After that, we can compute the spectral radiance at the exit of integral sphere by Plank formula. So we not only complete the calibration of the integral sphere source, but also have the integral sphere source trace to the blackbody simultaneously. From the result analysis,we think this method is exact enough for the calibration about the spectral radiation of the integral sphere source.
机译:校准成像光谱仪时,必须使积分球源跟踪到标准灯。但是标准灯首先需要被黑体校准。在本文中,我们使用光谱仪的专有光谱响应将积分球源迹线直接跟踪到黑体。在实验过程中,分别通过测量1000℃黑体和在一定色温下的积分球体的光谱辐射,分别获得了700nm〜900nm范围内200nm〜1100nm光谱仪的两个光谱响应。理论上,利用两个光谱响应的一致性,我们获得了积分球体光源的等效色温。之后,我们可以通过Plank公式计算积分球出口处的光谱辐射率。因此,我们不仅要完成积分球源的校准,而且还要使积分球源迹线同时到达黑体。从结果分析来看,我们认为该方法对于积分球源光谱辐射的校准足够准确。

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