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Computed-tomography imaging spectropolarimeter (CTISP).

机译:计算机断层扫描成像光谱仪(CTISP)。

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摘要

A complete Stokes imaging spectropolarimeter has been developed based on the principles of computed-tomography, spectrometry and polarimetry. The Computed-Tomography Imaging SpectroPolarimeter (CTISP) is a polarization extension to the Computed Tomography Imaging Spectrometer (CTIS)1.; Imaging spectrometers estimate the object cube (x,y, λ), whose smallest subdivision is a voxel, while Stokes imaging spectrometers estimate four Stokes object cubes (x,y, Sp(λ); p = 0,1,2,3), one for each Stokes parameter.; CTISP uses a two-dimensional disperser to diffract the image in the field stop into a 5-by-5 array of diffraction orders. As in computed tomography, each focal plane array (FPA) pixel effectively integrates a different path through the object cube, and when all pixels are recorded, a significant portion of the object cube's information is obtained. The frequency space representation of the object cube, however, indicates that two conical regions of information are not recorded, thereby limiting the reconstruction accuracy.; CTISP scans only in the polarization domain (not spectral or spatial domains), acquiring four FPA frames, one behind each of the four polarization analyzers. Currently, CTISP's resolution is 33 by 33 spatially over a 3.5 degrees full angle field of view with 16 spectral bands of 20nm width covering 440nm–740nm.; CTISP acquisition is modeled using the linear imaging equation ga=Ha fa+x a , which is inverted using the iterative expectation-maximization algorithm to solve for fa , the object cube as seen through analyzer a . The recorded diffraction images ga and the empirically determined calibration matrices Ha , are each acquired using analyzer a . The nth voxel reconstruction result is extracted from each of the four fa vectors to form a four element vector f&d4;&ar; n which is then multiplied by the inverse of the voxel characteristic matrix Wn to obtain the estimate of the Stokes vector S&d4;n . Wn is derived from the four Ha matrices.; 1M. R. Descour, E. L. Dereniak, “Computed-tomography imaging spectrometer: experimental calibration and reconstruction results”, Applied Optics, 34, No 22, pp. 4817–4828 (August 1995).
机译:基于计算机断层扫描,光谱学和极化仪的原理,已经开发出了完整的斯托克斯成像光谱旋光仪。计算机断层扫描成像光谱仪(CTISP)是计算机断层扫描成像光谱仪(CTIS) 1 的偏振扩展。成像光谱仪估计对象立方体(x,y,λ),其最小细分为体素,而Stokes成像光谱仪估计四个Stokes对象立方体(x,y, S p (λ); p = 0、1、2、3),每个Stokes参数一个。 CTISP使用二维分散器将场阑中的图像衍射成5×5衍射级阵列。如在计算机断层扫描中一样,每个焦平面阵列(FPA)像素有效地整合了通过对象多维数据集的不同路径,并且当记录所有像素时,将获得对象多维数据集信息的重要部分。然而,对象立方体的频率空间表示指示未记录两个圆锥形的信息区域,从而限制了重建精度。 CTISP仅在极化域(而不是光谱域或空间域)中扫描,获取四个FPA帧,在四个偏振分析仪中的每一个后面。目前,CTISP的分辨率在3.5度全视角范围内具有33 x 33的空间分辨率,并具有16个20nm宽度的光谱带,覆盖440nm至740nm。使用线性成像方程 g a = H建模CTISP采集 a f a + x a math>,使用迭代期望最大化算法对它进行求逆,以求解 f a ,即通过分析器 a 看到的对象立方体。记录的衍射图像 g a 和根据经验确定的校准矩阵 H a 每个都是使用分析器 a 获取的。从四个 f a 的每一个中提取 n 体素重建结果inf> 向量形成一个四元素向量 f &d4; < / ac> &ar; n ,然后乘以体素的倒数特征矩阵 W n 以获得斯托克斯矢量的估计 S &d4; n W n 源自四个 H a 矩阵。 1 M。 R. Descour,EL Dereniak,“计算机断层成像成像光谱仪:实验校准和重建结果”, Applied Optics 34 ,第22期,第4817–4828页(八月1995)。

著录项

  • 作者

    Miles, Brian Herndon.;

  • 作者单位

    The University of Arizona.;

  • 授予单位 The University of Arizona.;
  • 学科 Physics Optics.; Physics Astronomy and Astrophysics.; Engineering Electronics and Electrical.
  • 学位 Ph.D.
  • 年度 1999
  • 页码 187 p.
  • 总页数 187
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 光学;天文学;无线电电子学、电信技术;
  • 关键词

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