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首页> 外文期刊>International journal of remote sensing >Image-based spacecraft pointing model using single-bank dual-band registration
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Image-based spacecraft pointing model using single-bank dual-band registration

机译:基于单库双频配准的基于图像的航天器指向模型

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摘要

The growing interest in the development of small satellites and the demand for high-resolution imaging has made the pointing and drift rate requirements of a satellite more stringent. To achieve high pointing accuracy, star sensors can be used, but their size and weight are too large for small satellites. The need for keeping the overall cost of the spacecraft down and still achieve adequate pointing accuracies has provoked the development of relatively inexpensive and high-performance attitude systems that can provide competitive pointing accuracies during imaging operations. In order to realize such a system, this research describes a novel approach for finding the attitude of a satellite at any arbitrary rotation by using inter-band offsets from a single multi-spectral imager (MSI). For Earth observational imagery, UK Disaster Monitoring Constellation Earth-pointing MSI is used. This research focuses on the potential use of a narrow angle between the bands of a pushbroom sensor for determining the attitude of a spacecraft. The technique investigated does not require ground control points or knowledge of any ground features, but rather estimates the orientation of the platform through analysis of perspective and timing-based distortions between images. These distortions are assumed translational and affine in nature, with two-dimensional shifts being extracted from imagery using a Singular Value Decomposition-based registration scheme. In order to better understand the effect of attitude on imagery, a model was developed for predicting inter-band shifts given an attitude. This was then used to estimate the shifts between imagery at nominal attitude and given a series of simulated manoeuvres. Several simulations have shown that the row and column offsets represented a straight line. Hence, we expressed the row and column shifts in terms of straight line parameters. These geometric attributes are then represented in terms of Euler axis/angle to find the mapping for the elements of the general rotation matrix. Once the mapping is computed for the elements of the rotation matrix, we used the standard equations to determine the angle of rotation and Euler axis. The accuracy of attitude estimates depends on the magnitude of angular separation between the cameras, orientation of spacecraft, sensor resolution, image texture, and image registration method. The technique proposed in this study may however be applied to any satellite with pushbroom sensors that have a discernable along track separation and sufficient overlap.
机译:对小型卫星发展的兴趣日益增长,对高分辨率成像的需求也使得对卫星的指向和漂移速率的要求更加严格。为了获得较高的指向精度,可以使用星形传感器,但是它们的大小和重量对于小型卫星而言太大。为了降低航天器的总体成本并仍然获得足够的指向精度,这种需求促使开发出相对廉价且高性能的姿态系统,该系统可以在成像操作中提供具有竞争力的指向精度。为了实现这样的系统,本研究描述了一种新颖的方法,该方法通过使用来自单个多光谱成像器(MSI)的带间偏移来查找任意旋转的卫星的姿态。对于地球观测图像,使用了英国灾难监测星座地球指向MSI。这项研究的重点是在推扫帚传感器的各条带之间使用窄角度来确定航天器的姿态。所研究的技术不需要地面控制点或任何地面特征的知识,而是通过分析视角和图像之间基于时间的失真来估计平台的方向。这些失真本质上被假定为平移和仿射的,其中使用基于奇异值分解的配准方案从图像中提取了二维偏移。为了更好地了解态度对图像的影响,开发了一种模型,用于预测给定态度下的带间偏移。然后将其用于估计名义姿态和给定的一系列模拟动作之间的图像偏移。若干模拟表明,行和列偏移量表示一条直线。因此,我们用直线参数表示行和列的移动。然后用欧拉轴/角度表示这些几何属性,以找到通用旋转矩阵元素的映射。一旦为旋转矩阵的元素计算了映射,我们就可以使用标准方程式来确定旋转角度和欧拉轴。姿态估计的准确性取决于相机之间的角度间隔大小,航天器的方向,传感器分辨率,图像纹理和图像配准方法。然而,这项研究中提出的技术可以应用于带有推扫传感器的任何卫星,这些卫星在轨道间距和可重复性方面都可辨别。

著录项

  • 来源
    《International journal of remote sensing》 |2014年第22期|7583-7613|共31页
  • 作者单位

    Natl Univ Sci & Technol, Sch Elect Engn & Comp Sci, Dept Comp, Islamabad, Pakistan;

    Univ Surrey, Surrey Space Ctr, Guildford GU2 7XH, Surrey, England;

    Natl Univ Sci & Technol, Sch Elect Engn & Comp Sci, Dept Comp, Islamabad, Pakistan;

    Natl Univ Sci & Technol, Sch Elect Engn & Comp Sci, Dept Comp, Islamabad, Pakistan;

    Natl Univ Sci & Technol, Sch Elect Engn & Comp Sci, Dept Comp, Islamabad, Pakistan;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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