Chinese Journal of Lasers, Volume. 50, Issue 13, 1310004(2023)

Study on Tomography Performance of Multi-Conjugated Adaptive Optics Affected by Configuration of Sodium Laser Guide Star Constellation

Jian Huang1 and Gongchang Wang2、*
Author Affiliations
  • 1Chongqing Key Laboratory of Manufacturing Equipment Mechanism Design and Control, School of Mechanical Engineering, Chongqing Technology and Business University, Chongqing 400067, China
  • 2No. 32037 Unit of PLA, Yaoan, Yunnan 675300, China
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    Figures & Tables(11)
    Principle of MCAO system based on sodium LGSs. (a) Schematic diagram for two-layer turbulent tomography by MCAO system with three sodium LGSs constellation; (b) transformation of coordinates between footprint and meta-pupil, where xoy is for meta-pupil coordinates and x'o'y' is for footprint coordinates
    Gray map of projection matrix for three sodium LGSs constellation
    Simulated results of wavefront reconstruction with two layers of atmospheric turbulence and three sodium LGSs through tomography. Upper row for ground layer turbulence and lower row for high layer turbulence. (a), (d) Initial distorted wavefront; (b), (e) reconstructed wavefront through tomography; (c), (f) residual error
    SR map obtained by MCAO system with three sodium LGSs, with yellow pentagrams representing sodium LGSs
    Performance evolution of 500 frames for MCAO system with three sodium LGSs during 1 s
    Constellations of sodium LGSs with different numbers and located at different positions. (a) 3+1; (b) 4; (c) 4+1; (d) 5; (e) 5+1; (f) 6
    SR maps obtained by MCAO systems for sodium LGS constellations with different numbers and configurations, with yellow pentagrams representing sodium LGSs. (a) 3+1; (b) 4; (c) 4+1; (d) 5; (e) 5+1; (f) 6
    Mean values of SR and STD obtained by MCAO systems for sodium LGS constellations with different numbers and configurations
    Influence of zenith angle of sodium LGSs on performance of MCAO system
    Influence of zenith angle of sodium LGSs on uniformity of MCAO system
    • Table 1. Main parameters for simulation

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      Table 1. Main parameters for simulation

      TypeVariableValueDescription
      Atmospherer0 /cm8Fried parameter(@550 nm)
      Fsampling /Hz500Sampling frequency
      Hi /km0, 8Turbulent layer altitude
      Si0.7, 0.3Turbulent layer relative strength
      TelescopeD /m10Diameter of telescope
      θFOV /(′)1Field of view
      λH bandObservation band
      θT /(°)0Zenith angle of telescope
      Sodium LGSHLGS /km90Altitude of LGSs
      n3Number of LGSs
      RLGS /(″)41.459Zenith angle of each LGS
      Azimuth angle /(°)0, 120, 240Azimuth angle of each LGS
      λLGS /nm589.159Wavelength of sodium LGS
      M0Magnitude of LGS
      WFSd /m0.4Diameter of sub-aperture of WFS
      Sub-aperture resolution /pixel10×10Number of pixel in each sub-aperture
      Zernike order105Order for Zernike polynomials decomposition
      K25×25Sub-aperture number of WFS
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    Jian Huang, Gongchang Wang. Study on Tomography Performance of Multi-Conjugated Adaptive Optics Affected by Configuration of Sodium Laser Guide Star Constellation[J]. Chinese Journal of Lasers, 2023, 50(13): 1310004

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    Paper Information

    Category: remote sensing and sensor

    Received: Dec. 21, 2022

    Accepted: Feb. 8, 2023

    Published Online: Jun. 27, 2023

    The Author Email: Wang Gongchang (wh-99@126.com)

    DOI:10.3788/CJL221553

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