Welsh B M, Koeffler S C
Appl Opt. 1994 Jul 20;33(21):4880-8. doi: 10.1364/AO.33.004880.
In the theory of atmospheric turbulence, the strength of the spatial variations of the index of refraction n is proportional to a parameter known as the atmospheric-structure constant. The atmosphericstructure constant is denoted C(2)(n)(z) and is a function of position along the optical path z. The characteristics of the temporal variations of the index of refraction are related to both C(2)(n)(z) and to the transverse wind velocity V(z). Current optical techniques for remotely sensing C(2)(n)(z) and V(z) rely primarily on the spatial or temporal cross-correlation properties of the intensity of the optical field. In the remote-sensing technique proposed here, we exploit the correlation properties of the wave-front slope measured from two point sources to obtain profiles of C(2)(n)(z) and V(z). The two sources are arranged to give crossed optical paths. The geometry of the crossed paths and the characteristics of the wave-front slope sensor determine the achievable resolution. The signal-to-noise ratio calculationsindicate the need for multiple measurements to obtain useful estimates of the desired quantities.
在大气湍流理论中,折射率n的空间变化强度与一个被称为大气结构常数的参数成正比。大气结构常数用C₂(n)(z)表示,是沿光路z位置的函数。折射率的时间变化特性与C₂(n)(z)以及横向风速V(z)都有关系。当前用于遥感测量C₂(n)(z)和V(z)的光学技术主要依赖于光场强度的空间或时间互相关特性。在此提出的遥感技术中,我们利用从两个点源测量的波前斜率的相关特性来获取C₂(n)(z)和V(z)的剖面图。这两个源被布置成提供交叉光路。交叉光路的几何结构和波前斜率传感器的特性决定了可实现的分辨率。信噪比计算表明需要进行多次测量才能获得所需量的有用估计值。