Infrared and Laser Engineering, Volume. 53, Issue 5, 20240098(2024)

Research progress and prospects of suppressing atmospheric turbulence with optical pin beams (cover paper·invited)

Chao Liu1,2,3,4, Rong Wang1,2,3,4, Bin Lan1,2,3, Xueying Li1,2,3, Kaihe Zhang1,2,3, Tianjun Dai1,2,3, and You Zhang1,2,3,4
Author Affiliations
  • 1Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China
  • 2National Laboratory on Adaptive Optics, Chengdu 610209, China
  • 3Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu 610209, China
  • 4University of Chinese Academy of Sciences, Beijing 100049, China
  • show less
    Figures & Tables(14)
    Principle diagram of optical pin beams formation[10]
    Far field spot image after propagating over a distance of 1 km in open areas. (a) Spot image of Gaussian beams; (b) Spot image of optical pin beams[10]
    The propagation image of the optical pin beams (a1) γ = 1.5, (b1) γ = 1 and (c1) γ = 0.5 the longitudinal strength distribution in the y-z plane obtained by 0.5; (a2), (b2) and (c2) depict the transverse intensity maps of the light spot captured at a plane z= 200 mm[11]
    Experimental setup and result diagram. (a) Experimental setup diagram; (b1), (c1) Experimental results of longitudinal intensity distribution of optical pin beams and abruptly autofocusing beams in the y-z plane; (b2), (c2) Lateral intensity diagram at the starting position; (b3), (c3) Lateral intensity diagram measured near the peak intensity plane; (b4), (c4) Lateral intensity diagram measured after 500 mm propagation; (b5), (c5) Phase mask loaded into the SLM device[11]
    Power loss diagram for Gaussian beams, focused Gaussian beams and optical pin beams transmission at 0.1-0.8 m[14]
    BER performance and eye diagrams for a Gaussian beams and optical pin beams. (a) z = 0.45 m; (b) z = 0.8 m[14]
    Experimental setup diagram for the generation and detection of VOPB[17]
    OAM spectra of the receiving surface in turbulent atmosphere at different receiving apertures R. (a)-(c) OAM spectrum of POVB; (d)-(f) OAM spectrum of Gaussian vortex beams[19]
    Far-field images of LG vortex beams and POVB[20]
    The mean intensity centroid position offset and jitter diagram of POVB and LVB[20]
    Comparison of transmission characteristics between SOB and Gaussian beams. (a) The beam pattern of SOB (upper) and Gaussian beams (lower) at a transmission distance of −6 cm to 6 cm; (b) Diagram of changes in beam radius for SOB and Gaussian beams at transmission distances of −12 cm to 12 cm[21]
    Comparison of effects between SOB and Gaussian beams before and after turbulence. (a) Side view of beam profile of SOB and Gaussian beams passing through a water tank without turbulence; (b) Spot of SOB after passing through turbulent water; (c) Spot of Gaussian beams after passing through turbulent water; (d) Distribution of light intensity when Gaussian beams and SOB transmission distance is 0-20 mm; (e) Relative intensity fluctuation of Gaussian beams and SOB in 0-20 s[21]
    Experimental optical path diagram of SOB and Gaussian beams transmitted through turbulence[22]
    Comparison before and after optimization. (a) Experimental diagram of SOB before optimization; (b) Experimental diagram of optimized SOB; (c) Measurement of spot radius at different transmission distances of SOB[23]
    Tools

    Get Citation

    Copy Citation Text

    Chao Liu, Rong Wang, Bin Lan, Xueying Li, Kaihe Zhang, Tianjun Dai, You Zhang. Research progress and prospects of suppressing atmospheric turbulence with optical pin beams (cover paper·invited)[J]. Infrared and Laser Engineering, 2024, 53(5): 20240098

    Download Citation

    EndNote(RIS)BibTexPlain Text
    Save article for my favorites
    Paper Information

    Category:

    Received: Mar. 4, 2024

    Accepted: --

    Published Online: Jun. 21, 2024

    The Author Email:

    DOI:10.3788/IRLA20240098

    Topics