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Calculating Viewing Angles Pixel by Pixel in Optical Remote Sensing Satellite Imagery Using the Rational Function Model

机译:使用Rational函数模型计算光遥感卫星图像中的像素的视角像素

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摘要

In studies involving the extraction of surface physical parameters using optical remote sensing satellite imagery, sun-sensor geometry must be known, especially for sensor viewing angles. However, while pixel-by-pixel acquisitions of sensor viewing angles are of critical importance to many studies, currently available algorithms for calculating sensor-viewing angles focus only on the center-point pixel or are complicated and are not well known. Thus, this study aims to provide a simple and general method to estimate the sensor viewing angles pixel by pixel. The Rational Function Model (RFM) is already widely used in high-resolution satellite imagery, and, thus, a method is proposed for calculating the sensor viewing angles based on the space-vector information for the observed light implied in the RFM. This method can calculate independently the sensor-viewing angles in a pixel-by-pixel fashion, regardless of the specific form of the geometric model, even for geometrically corrected imageries. The experiments reveal that the calculated values differ by approximately 10−40 for the Gaofen-1 (GF-1) Wide-Field-View-1 (WFV-1) sensor, and by ~10−70 for the Ziyuan-3 (ZY3-02) panchromatic nadir (NAD) sensor when compared to the values that are calculated using the Rigorous Sensor Model (RSM), and the discrepancy is analyzed. Generally, the viewing angles for each pixel in imagery are calculated accurately with the proposed method.
机译:在涉及使用光学遥感卫星图像提取表面物理参数的研究中,必须知道太阳传感器几何形状,特别是对于传感器观察角度。然而,虽然传感器观察角的逐像素获取对许多研究具有至关重要的重要性,但是用于计算传感器观察角度的现有算法仅在中心点像素上聚焦或者是复杂的并且不公知的算法。因此,本研究旨在提供一种简单且一般的方法来估计传感器观察角度像素的像素。 Rational函数模型(RFM)已经广泛用于高分辨率卫星图像,因此提出了一种方法,用于基于在RFM中隐含的观察光的空间 - 矢量信息来计算传感器观察角度。这种方法可以以像素 - 逐个像素的方式独立地计算传感器观看角度,而不是几何模型的特定形式,即使对于几何校正的成像。实验表明,计算的值对于高芬-1(GF-1)宽场 - View-1(WFV-1)传感器的差异约为10-40,并为Ziyuan-3(ZY3)〜10-70 -02)与使用严格的传感器模型(RSM)计算的值相比,Panchromatic Nadir(NAD)传感器,分析差异。通常,用所提出的方法准确地计算图像中的每个像素的观察角度。

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