• Acta Optica Sinica
  • Vol. 43, Issue 6, 0636001 (2023)
Shengnan Chen**, Chunyan Wang***, Hao Sun, and Huilin Jiang*
Author Affiliations
  • School of Opto-Electronic Engineering, Changchun University of Science and Technology, Changchun 130033, Jilin, China
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    DOI: 10.3788/AOS222100 Cite this Article Set citation alerts
    Shengnan Chen, Chunyan Wang, Hao Sun, Huilin Jiang. Method of Far-Field Phase Noise Suppression for Space Gravitational-Wave Detection Telescope[J]. Acta Optica Sinica, 2023, 43(6): 0636001 Copy Citation Text show less
    Schematic diagram of telescope system
    Fig. 1. Schematic diagram of telescope system
    Normalized distributions of received energy. (a) Intensity distribution curve; (b) intensity distribution
    Fig. 2. Normalized distributions of received energy. (a) Intensity distribution curve; (b) intensity distribution
    Comparison of analytical and numerical calculations of WE (α,β)
    Fig. 3. Comparison of analytical and numerical calculations of WE (α,β)
    WE (α,β) of System1 and System2. (a) System1; (b) System2
    Fig. 4. WE (α,β) of System1 and System2. (a) System1; (b) System2
    δfar(α, β) of System1 and System2. (a) δfar(α, β) in sagittal and tangential planes; (b) δfar(α, β) of System1 and System2
    Fig. 5. δfar(α, β) of System1 and System2. (a) δfar(α, β) in sagittal and tangential planes; (b) δfar(α, β) of System1 and System2
    TelescopeMirrorR /mmky /mmz /mmTilt /(°)
    Telescope in System1M1--000
    1410.501.000-
    M2-66.21-0673.65
    1.189
    M3-564.69-0165.1110.773
    M4746.09--79.7514.137
    80.36
    Telescope in System2M1--000
    1410.781.000
    M2-66.15-0-0
    1.176673.79
    M3-577.70-0193.1610.809
    M4816.85--116.8814.011
    78.95
    Table 1. Structural parameters of telescopes in System1 and System2
    TermSystem1System2
    C4-2.55463×10-2λ-3.61899×10-5λ
    C5-9.37489×10-2λ6.59153×10-3λ
    C8-7.98534×10-2λ-1.45964×10-1λ
    C96.15331×10-3λ-4.14483×10-4λ
    C118.99012×10-4λ2.91833×10-3λ
    C12-1.36633×10-3λ-2.02830×10-3λ
    C157.37880×10-4λ1.33327×10-3λ
    σw0.0499λ0.0517λ
    Table 2. Ci and corresponding σw of System1 and System2
    Shengnan Chen, Chunyan Wang, Hao Sun, Huilin Jiang. Method of Far-Field Phase Noise Suppression for Space Gravitational-Wave Detection Telescope[J]. Acta Optica Sinica, 2023, 43(6): 0636001
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