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首页> 外文期刊>Selected Topics in Applied Earth Observations and Remote Sensing, IEEE Journal of >A Study of Wind Direction Effects on Sea Surface Specular Scattering for GNSS-R Applications
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A Study of Wind Direction Effects on Sea Surface Specular Scattering for GNSS-R Applications

机译:风向对GNSS-R应用海面镜面散射的影响研究

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A modeling study investigating the influence of wind direction on spaceborne global navigation satellite system reflectometry (GNSS-R) near-specular observations of the sea surface is reported. The study first focuses on a purely specular geometry under plane wave incidence, for which it is shown using the theorem of reciprocity and reflection symmetry that up-down wind variations are identically zero. It is also shown that “single-scattering” approximations of rough surface scattering predict no variations with wind direction of any kind for a purely specular geometry, while higher order approximations (such as the second-order small-slope approximation) can predict up/cross wind differences. Examples of these variations are reported and found to be small. Because the delay doppler maps (DDMs) measured in GNSS-R include some nonspecular contributions even for “specular” portions of the DDM, the second part of the study performs an examination of near-specular DDM variations with wind direction using the widely used geometrical optics approximation of surface scattering for a surface described with the non-Gaussian Cox–Munk slope probability density function. Variations with wind direction of the normalized radar cross section (NRCS) mapped onto the surface are examined, and again, it is shown that these variations are small for surface portions contributing to the near-specular portion of the DDM. In addition, it is shown that the dependencies of the bistatic NRCS on wind direction are such that differing portions of the surface “glistening zone” have differing phase shifts in their dependence on wind direction, causing the wind dependencies of the final near-specular DDM to be negligible. The final results of the study suggest that any wind direction dependence in spaceborne GNSS-R should be sought only in portions of the DDM away from the specular region. These results provide information to guide analyses of the wind direction information available in current GNSS-R missions such as TDS-1 and Cyclone Global Navigation Satellite System.
机译:报告了一项模型研究,该研究调查了风向对海面近镜观测的星载全球导航卫星系统反射法(GNSS-R)的影响。这项研究首先关注平面波入射下的纯镜面几何,并通过互易和反射对称定理证明了上下风的变化完全为零。还表明,对于纯镜面几何,粗糙表面散射的“单散射”近似值不会预测任何风向的变化,而更高阶的近似值(例如二阶小斜率近似值)可以预测向上/逆风差异。报告了这些变化的示例,发现很小。由于在GNSS-R中测得的延迟多普勒图(DDM)甚至对DDM的“镜面”部分都包含了一些非镜面反射,因此研究的第二部分使用广泛使用的几何学方法对风向近镜面DDM变化进行了检查。用非高斯Cox-Munk斜率概率密度函数描述的表面的表面散射的光学近似。研究了映射到表面的归一化雷达横截面(NRCS)随风向的变化,再次表明,这些变化对于有助于DDM接近镜面部分的表面部分很小。此外,还显示了双基地NRCS对风向的依赖性,使得表面“闪耀区”的不同部分在其对风向的依赖性方面具有不同的相移,从而导致了最终近镜面DDM的风依赖性可以忽略不计。研究的最终结果表明,应仅在DDM远离镜面反射区域的部分中寻找星空GNSS-R中任何与风向相关的问题。这些结果为指导分析当前GNSS-R任务(例如TDS-1和旋风全球导航卫星系统)中可用的风向信息提供了信息。

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