对地观测航天器偏航偏差模型

A. Sinha, M. Zaheer, Sonia Behal
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引用次数: 0

摘要

大多数遥感航天器携带的有效载荷是交错CCD配置(奇数和偶数像素线性分布在2行)。主要要求是两个像素阵列捕获相同的扫描行以实现平滑成像。然而,由于两个CCD阵列到达成像线上的时间差,由于地球在这段时间内旋转,两个阵列无法扫描到同一条线。由于地球表面的大圆由于其扁性和非对称结构,其半径是可变的,因此在考虑球形地球模型时,由于存在大量的谐波,偏转偏差作为地球自转补偿的计算非常复杂。本文考虑平坦地球模型,推导了星下纬度的偏航偏置(绕最低点轴旋转)模型,该模型适用于近地轨道航天器数百米左右的条带覆盖范围。该模型简单易懂,利用航天器的轨道几何特性和基本的三角恒等式推导。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Yaw Bias Model for Earth Observation Spacecrafts
Most of the remote sensing spacecrafts carry payload with staggered CCD configuration (odd and even pixels spread linearly in 2 rows). Prime requirement is to capture the same line of scan by both arrays of pixels for smooth imaging. However, due to time difference in the arrival of the two CCD arrays over imaging line, the same line can’t be scanned by the two arrays as the earth has rotated in that duration. As, radius of the greater circle on the surface of earth is variable due to its oblateness and non symmetric structure and so computation of yaw bias as a compensation for earth’s rotation is very complicated due to large number of harmonics, if spherical earth model is considered. In this paper, yaw bias (rotation about nadir axis) model with respect to sub satellite latitude is derived, considering flat earth model which is very well valid for low earth orbit spacecrafts with swath coverage of about few hundred meters. The model is simple, easy to understand and is derived using orbit geometry of the spacecraft and basic trigonometric identities.
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