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    Area of Science:

    • Optical engineering
    • Telescope instrumentation
    • Structural analysis

    Background:

    • The Thirty Meter Telescope's linear atmospheric dispersion corrector (LADC) uses large prisms.
    • Prism support structures cause gravitational and reaction forces, leading to surface deformation.
    • Current open-loop analysis methods are inefficient and expertise-dependent.

    Purpose of the Study:

    • To develop a more efficient closed-loop integrated model analysis optimization method.
    • To reduce prism surface deformation in the LADC.
    • To improve the optimization process for telescope optical components.

    Main Methods:

    • Implemented a closed-loop integrated model analysis optimization method.
    • Integrated interface programs between analysis tools.
    • Utilized Optimal Latin Hypercube Design (Opt LHD) and Particle Swarm Optimization (PSO) algorithms.

    Main Results:

    • Reduced analysis time from one week to two days.
    • Decreased optical surface deformation by 49.3% (155.0 nm to 78.6 nm) under specific conditions.
    • Achieved a 62.5% reduction in deformation (289.1 nm to 108.4 nm) under different conditions.

    Conclusions:

    • The closed-loop method significantly enhances optimization efficiency.
    • The optimized prism support structure substantially reduces optical surface deformation.
    • This approach offers a more reliable and effective solution for optical instrument design.