Chinese Optics, Volume. 15, Issue 4, 740(2022)

Film thickness uniformity of deep ultraviolet large aperture aspheric mirror

Yong-gang PAN1, Zhao-wen LIN1、*, Ben WANG1,3, and Xiu-hua FU1,2
Author Affiliations
  • 1Zhongshan Institute of Changchun University of Science and Technology, Zhongshan 528437, China
  • 2School of Optoelectronic Engineering, Changchun University of Science and Technology, Changchun 130022, China
  • 3Zhongshan Gilion Optoelectronics Technology Co., Ltd., Zhongshan 528437, China
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    Figures & Tables(13)
    Schematic diagram of the rotational planetary mechanism
    The flow chart of film thickness simulation
    The plot of coordinate transformation
    Schematic diagram of the OTFC-1300 revolution planetary instrument
    The relative film thickness distributions of (a) HfO2 and (b) SiO2
    The clip diagram
    The sketch of the baffle shape
    The film thickness distribution
    Actual tested spectral curves
    The surface topography date of the mirror
    • Table 1. The orbit of revolution of a planetary structure

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      Table 1. The orbit of revolution of a planetary structure

      GeometryTrajectory
      Coordinates of any point on the substrate holder${x_{{p} } } = D\sin\; {\omega _1}t + \rho \sin \;({\omega _1}t + {\omega _2}t)$${y_{{p} } } = D\cos \;{\omega _1}t + \rho \cos\; \left( { {\omega _1}t + {\omega _2}t} \right)$${\textit{z}_p} = H$
      Evaporation distance$\sqrt { { {\left( { {x_{ {p} } } } \right)}^2} + { {\left( { {y_{ {p} } } - L} \right)}^2} + { {\left( { {\textit{z}_{ {p} } } } \right)}^2} }$
      Evaporation angle$\mathrm{cos}\;\varphi=\dfrac{\boldsymbol{D}\cdot\boldsymbol{PP_{{\rm{s}}} } }{\left|\boldsymbol{D}\right|\left|\boldsymbol{PP_{{\rm{s}}} }\right|}$
      Projected angle$\mathrm{cos}\;\theta =\dfrac{\boldsymbol{D}\cdot\boldsymbol{PP_{ {\rm{s} } } } }{\left|\boldsymbol{D}\right|\left|\boldsymbol{PP_{ {\rm{s} } } }\right|}$
    • Table 2. The technical parameters of the large aspherical mirror

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      Table 2. The technical parameters of the large aspherical mirror

      ParametersIndicators
      SubstrateJGS1
      Angle of incidence /(°)0
      Spectral range /nm230~300
      Reflectance≥97.5%
      Heterogeneity≤0.5%
    • Table 3. The process parameters of thin film preparation

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      Table 3. The process parameters of thin film preparation

      MaterialIon source voltage /V Ion source current /mA Ion source O2 gas flow /ml·min−1O2 gas flow /ml·min−1Substrate temperature/°CDeposition rate /nm·s−1
      HfO250040050502000.12
      SiO25004005002000.8
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    Yong-gang PAN, Zhao-wen LIN, Ben WANG, Xiu-hua FU. Film thickness uniformity of deep ultraviolet large aperture aspheric mirror[J]. Chinese Optics, 2022, 15(4): 740

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    Paper Information

    Category: Original Article

    Received: Jan. 6, 2022

    Accepted: Apr. 6, 2022

    Published Online: Sep. 6, 2022

    The Author Email:

    DOI:10.37188/CO.2022-0005

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