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Design and optimization of a dispersive unit based on cascaded volume phase holographic gratings

机译:基于级联体相全息光栅的色散单元设计与优化

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摘要

We describe a dispersive unit consisting of cascaded volume-phase holographic gratings for spectroscopic applications. Each of the gratings provides high diffractive efficiency in a relatively narrow wavelength range and transmits the rest of the radiation to the 0th order of diffraction. The spectral lines formed by different gratings are centered in the longitudal direction and separated in the transverse direction due to tilt of the gratings around two axes. We consider a technique of design and optimization of such a scheme. It allows to define modulation of index of refraction and thickness of the holographic layer for each of the gratings as well as their fringes frequencies and inclination angles. At the first stage the gratings parameters are found approximately using analytical expressions of Kogelnik's coupled wave theory. Then each of the grating starting from the longwave sub-range is optimized separately by using of numerical optimization procedure and rigorous coupled wave analysis to achieve a high diffraction efficiency profile with a steep shortwave edge. In parallel such targets as ray aiming and linear dispersion maintenance are controlled by means of ray tracing. We " demonstrate this technique on example of a small-sized spectrograph for astronomical applications. It works in the range of 500-650 run and uses three gratings covering 50 nm each. It has spectral resolution of 6130-12548.Obtaining of the asymmetrical efficiency curve is shown with use of dichromated gelatin and a photopolymer. Change of the curve shape allows to increase filling coefficient for the target sub-range up to 2.3 times.
机译:我们描述了由级联的体积相全息光栅组成的色散单元,用于光谱应用。每个光栅在相对窄的波长范围内提供高衍射效率,并将其余的辐射透射到衍射的0级。由于光栅围绕两个轴的倾斜,由不同光栅形成的光谱线在纵向方向上居中并且在横向方向上分开。我们考虑一种设计和优化这种方案的技术。它允许定义每个光栅的折射率和全息层厚度的调制以及它们的条纹频率和倾斜角。在第一阶段,大致使用Kogelnik耦合波理论的解析表达式找到光栅参数。然后,通过数值优化程序和严格的耦合波分析分别优化从长波子范围开始的每个光栅,以实现具有陡峭短波边缘的高衍射效率曲线。平行地,诸如射线瞄准和线性色散维持的目标是通过射线追踪来控制的。我们在一个用于天文应用的小型光谱仪的示例中演示了该技术。该技术在500-650的范围内工作,并使用三个覆盖50 nm的光栅。其光谱分辨率为6130-12548。获得不对称效率使用重铬酸盐明胶和光敏聚合物显示曲线,曲线形状的变化可以将目标子范围的填充系数提高至2.3倍。

著录项

  • 来源
    《Holography: Advances and modern trends V》|2017年|102331l.1-102331l.10|共10页
  • 会议地点 Prague(CZ)
  • 作者单位

    Aix Marseille Univ, CNRS, LAM, Laboratoire d'Astrophysique de Marseille, Marseille, France, 38 Frederic Joliot-Curie, Marseille, France 13388,Kazan National Research Technical University named after A.N. Tupolev-KAI 10 K. Marx, Kazan, Russian Federation 420111;

    Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz, Russian Federation 369167;

    Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz, Russian Federation 369167;

    Kazan National Research Technical University named after A.N. Tupolev-KAI 10 K. Marx, Kazan, Russian Federation 420111;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    volume-phase holographic grating; diffraction efficiency; spectrograph; conical diffraction;

    机译:体相全息光栅;衍射效率光谱仪锥形衍射;
  • 入库时间 2022-08-26 13:45:43

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