4.6 Article

Influence of optical aperture sizes on aero-optical effects induced by supersonic turbulent boundary layers

Journal

OPTICS EXPRESS
Volume 31, Issue 12, Pages 19133-19145

Publisher

Optica Publishing Group
DOI: 10.1364/OE.491913

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With the increase of flight speed, aero-optical effects induced by the turbulent boundary layer near the optical window become increasingly significant. The influence of the optical aperture size on the aero-optical effects of supersonic (Mach 3.0) turbulent boundary layer (SPTBL) was studied, and the underlying mechanisms were analyzed. The results showed that the optical aperture size affects the beam jitter, beam offset, and beam spread, which are caused by turbulent structures of different scales.
With the increase of flight speed, aero-optical effects induced by the turbulent boundary layer near the optical window become increasingly significant. The density field of the supersonic (Mach 3.0) turbulent boundary layer (SPTBL) was measured by nano-tracer-based planar laser scattering technique, and the optical path difference (OPD) was obtained through ray-tracing method. The influence of the optical aperture size on the aero-optical effects of SPTBL was studied in detail, and the underlying mechanisms were analyzed from the perspective of the turbulent structure scales. The influence of the optical aperture on the aero-optical effects is mainly due to turbulent structures with different scales. The beam center jitter (sx over bar ) and offset (x over bar ) are mainly caused by turbulent structures larger than the optical aperture size, while the beam spread about the center (x & PRIME;2) is mainly caused by turbulent structures smaller than the optical aperture size. With the increase of optical aperture size, the proportion of turbulent structures larger than the optical aperture size decreases, which can suppress the beam jitter and the beam offset. Meanwhile, since the beam spread is primarily induced by small-scale turbulent structures with relatively strong density fluctuation intensity, the spread increases rapidly to its peak and then gradually stabilizes as the optical aperture size grows.& COPY; 2023 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement

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