应用于TerraSAR-X高分辨率聚光灯数据的PSInSAR大气相位屏幕估计

M. Even, A. Schunert, K. Schulz, U. Soergel
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引用次数: 4

摘要

十年前由Ferretti等人[1],[2],[3]发明的PSInSAR技术,同时也证明了它能够非常精确地测量表面变形。为了实现这一点,必须消除大气相屏(APS)的影响。我们研究了两组TerraSAR-X高分辨率射光数据在巴伐利亚的应用。我们的方法是将APS视为由相位斜坡,高度分层的部分和湍流成分组成。我们用克里格法估计了湍流分量。变差图显示了在较低分辨率下不可见的短距离状态。本文讨论了如何根据我们的数据选择合适的变异函数模型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Atmospheric phase screen-estimation for PSInSAR applied to TerraSAR-X high resolution spotlight-data
The PSInSAR technique, invented by Ferretti et. al. [1], [2], [3] ten years ago, meanwhile has proven it's capability for very precise measurement of surface deformations. To achieve this, the influence of the atmospheric phase screen (APS) has to be removed. We investigated the APS for two series of TerraSAR-X high resolution spotlight data of a scene in Bavaria. Our approach was to consider the APS as composed of a phase ramp, a part stratified with height and a turbulent component. We estimated the turbulent component via kriging. The variograms show for short distances a regime which is not visible for lower resolutions. In this paper we discuss the choice of appropriate variogram models with respect to our data.
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