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Vortex beam based more stable annular laser guide star

机译:基于涡旋光束更稳定的环形激光导航星

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We present an annular laser guide star (LGS) concept for large ground-based telescopes in this paper. The more stable annular LGS is generated by turbulence-resisted vortex beam. In the uplink, a vortex beam tends to wander more slightly than a Gaussian beam does in atmospheric turbulence. This may enable an annular LGS to wander more slightly than a traditional Gaussian beam generated LGS does, which would ease the burden of uplink tip-tilt mirror and benefit a dynamical closed-loop adaptive optics system. We conducted numerical simulation to validate the feasibility of this concept. And we have gotten 31% reduced variance of spot wandering of annular LGS. Besides, we set up a spatial light modulator based laser guide star simulator for beam propagation in turbulent atmosphere to experimentally test the annular LGS concept. Preliminary experimental results are given. To the best of our knowledge, it is the first time this concept is formulated.
机译:我们在本文中为大型地基望远镜提出了环形激光导航星(LGS)概念。通过湍流抵抗涡流束产生更稳定的环形LG。在上行,涡流波束倾向于比高斯光束在大气湍流中更略微漂移。这可以使环形LG略微比传统的高斯光束产生的LG略微漫游,这将缓解上行链路倾斜镜的负担并效益动态闭环自适应光学系统。我们进行了数值模拟以验证该概念的可行性。我们已经有31%的环形LG徘徊方差减少了31%。此外,我们建立了一种基于空间光调制器的激光导向星模拟器,用于湍流气氛中的光束传播,以实验测试环形LGS概念。给出了初步实验结果。据我们所知,这是第一次制定这个概念。

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