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Turbulent Thermal Blooming

机译:湍流热花

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摘要

Most system analyses of CW high-power lasers propagating in the atmosphere assume a simple additive linear relation of the impact of thermal blooming and optical turbulence in the atmosphere to the propagated laser beam spreading. In other words, both effects are treated as if they would follow Gaussian statistics in an RMS sense. While the statistics of optical propagation in a turbulent atmosphere can be modeled as Gaussian to first order, thermal blooming is a deterministic nonlinear optical phenomenon. To the best of our knowledge, there is no reason for adding linearly the beam spreading due to these two optical effects. In fact, assuming no interplay in the presence of a strong nonlinear optical interaction is counter-intuitive. As a result, we have performed extensive numerical Monte-Carlo optical wave-propagation simulations, >50,000 realizations, in the presence of thermal-blooming and atmospheric turbulence to varying degrees. During the propagation, the amplitude and the phase of a high power laser field are coupled by the interplay of diffraction, refractive turbulence and thermal blooming. In some cases, we have observed in our numerical experiments a strong coupling between turbulence and nonlinear thermal blooming.
机译:大多数在大气中传播的连续波高功率激光器的系统分析都假设大气中热起霜和光学湍流与传播的激光束扩散之间存在简单的线性关系。换句话说,这两种影响都被视为仿效RMS意义上的高斯统计。尽管可以将湍流中的光传播统计量建模为一阶高斯模型,但热起霜是确定性的非线性光学现象。据我们所知,由于这两种光学效应,没有理由线性地增加光束扩展。实际上,假设在强非线性光学相互作用下不存在相互作用是违反直觉的。结果,在不同程度的热花开和大气湍流的存在下,我们进行了广泛的蒙特卡洛光学波传播数值模拟,> 50,000个实现。在传播过程中,高功率激光场的振幅和相位通过衍射,折射湍流和热起霜的相互作用而耦合。在某些情况下,我们在数值实验中观察到了湍流和非线性热起霜之间的强耦合。

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