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Geometrical Calibration of an AOTF Hyper-spectral Imaging System

机译:AOTF超光谱成像系统的几何校准

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Optical aberrations present an important problem in optical measurements. Geometrical calibration of an imaging system is therefore of the utmost importance for achieving accurate optical measurements. In hyper-spectral imaging systems, the problem of optical aberrations is even more pronounced because optical aberrations are wavelength dependent. Geometrical calibration must therefore be performed over the entire spectral range of the hyper-spectral imaging system, which is usually far greater than that of the visible light spectrum. This problem is especially adverse in AOTF (AcoustoOptic Tunable Filter) hyper-spectral imaging systems, as the diffraction of light in AOTF filters is dependent on both wavelength and angle of incidence. Geometrical calibration of hyper-spectral imaging system was performed by stable caliber of known dimensions, which was imaged at different wavelengths over the entire spectral range. The acquired images were then automatically registered to the caliber model by both parametric and nonparametric transformation based on B-splines and by minimizing normalized correlation coefficient. The calibration method was tested on an AOTF hyper-spectral imaging system in the near infrared spectral range. The results indicated substantial wavelength dependent optical aberration that is especially pronounced in the spectral range closer to the infrared part of the spectrum. The calibration method was able to accurately characterize the aberrations and produce transformations for efficient sub-pixel geometrical calibration over the entire spectral range, finally yielding better spatial resolution of hyper-spectral imaging system.
机译:光学像差在光学测量中存在重要问题。因此,成像系统的几何校准对于实现精确的光学测量来说是至关重要的。在超光谱成像系统中,光学像差问题甚至更明显,因为光学像差是由波长相关的。因此,必须在超光谱成像系统的整个频谱范围内进行几何校准,该系统通常远远大于可见光光谱的频谱范围。该问题在AOTF(声光可调滤波器)超光谱成像系统中特别不利,因为AOTF滤波器中的光的衍射取决于波长和入射角。通过稳定的已知尺寸的稳定级来执行超光谱成像系统的几何校准,该尺寸在整个光谱范围内以不同波长成像。然后通过基于B样条曲线的参数和非参数变换以及通过最小化归一化相关系数来自动将所获取的图像自动登记到口径模型。在近红外光谱范围内的AOTF超光谱成像系统上测试了校准方法。结果表明,在频谱范围内的光谱范围特别明显的基本波长依赖性光学像差较近谱的红外部分。校准方法能够精确地表征像差并在整个光谱范围内产生用于有效的子像素几何校准的变换,最后产生更好的超光谱成像系统的空间分辨率。

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