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Modeling atmospheric precipitation impact on synthetic aperture radar imagery at X and Ka bands

机译:模拟大气降水对X和Ka波段合成孔径雷达图像的影响

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Spacebome synthetic aperture radars (SARs) operating at X-band and above allow observations of Earth surface at very high spatial resolution. Moreover, recent polarimetric SARs enable the complete characterization of target scattering and extinction properties. Nowadays several spaceborne X-band SAR systems are operative, and plans exist for systems operating at higher frequency bands (i.e. Ku, Ka and W). Although higher frequencies may have interesting and distinctive applications, atmospheric effects, especially in precipitating conditions, may affect the surface SAR response in both the signal amplitude and its phase, as assessed by numerous works in the last years. A valid tool to analyze and characterize the SAR response in these conditions is represented by forward modeling, where a known synthetic scenario, which is described by user-selected surface and atmospheric conditions, is considered. Thus, the SAR echoes corresponding to the synthetic scenarios are simulated using electromagnetic models. In this work a 3-D realistic polarimetric SAR response numerical simulator is presented. The proposed model framework accounts for the SAR slant observing geometry and it is able to characterize the polarimetric response both in amplitude and phase. In this work we have considered both X and Ka bands, thus exploring the atmospheric effects for the present and future polarimetric systems. The atmospheric conditions are simulated using the System for Atmospheric Modeling (SAM) which is an high-resolution mesoscale model. SAM is used to define the three-dimensional distribution of hydrometeors which are among the inputs used in the Hydrometeor Ensemble Scattering Simulator (HESS) T-Matrix which allow simulating the SAR signal due to the atmospheric component. The SAR surface component is, instead, simulated by a Semi Empirical Model (SEM) for bare-soils conditions and SEAWIND2 two-scale model for ocean surfaces. The proposed methodology has been applied in this work to assess the sensitivity of the considered frequency bands to different hydrometeor spatial distributions above some examples surface backgrounds.
机译:在X波段及以上工作的Spacebome合成孔径雷达(SAR)允许以非常高的空间分辨率观察地球表面。此外,最近的极化SAR能够完全表征目标散射和消光特性。如今,几个星载X波段SAR系统正在运行,并且存在在更高频段(即Ku,Ka和W)运行的系统的计划。尽管较高的频率可能具有有趣而独特的应用,但近年来的许多工作评估到,大气影响,尤其是在降水条件下,可能会影响信号幅值及其相位的表面SAR响应。前向建模代表了在这些条件下分析和表征SAR响应的有效工具,其中考虑了已知的合成情景,该情景由用户选择的地面和大气条件来描述。因此,使用电磁模型模拟了对应于合成情景的SAR回波。在这项工作中,提出了一种3D逼真的极化SAR响应数值模拟器。所提出的模型框架考虑了SAR倾斜观测的几何形状,并且能够表征振幅和相位上的极化响应。在这项工作中,我们同时考虑了X和Ka波段,从而探索了当前和未来极化系统的大气效应。大气条件是使用大气建模系统(SAM)进行模拟的,该系统是高分辨率的中尺度模型。 SAM用于定义水凝物的三维分布,这是在水凝体集合散射模拟器(HESS)T矩阵中使用的输入之一,该输入可以模拟由于大气成分而产生的SAR信号。 SAR表面分量由裸土条件的半经验模型(SEM)和海洋表面的SEAWIND2两尺度模型模拟。所提出的方法已用于这项工作中,以评估考虑的频带对某些示例表面背景之上的不同水凝物空间分布的敏感性。

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