机载红外传感器校准

M. O'Connor, L. Smith, L. Cheung
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引用次数: 0

摘要

仅给出摘要形式,如下。在机载平台上使用亚毫弧度红外测量传感器需要特殊的技术,以实现地球坐标与飞机坐标的参数精度。一般来说,机载平台包含一个GPS/INS系统,位于大约重心处。一般来说,传感器位于飞机的末端。因此,必须校准静态和动态(即挠曲)误差,以允许对空中目标的方位角和仰角进行精确的被动测量。传感器位置的高频动态弯曲通常由与传感器配置的第二个INS单元测量和校正。在不同的飞机机动条件下,由于飞机挠曲引起的静态偏移误差通常可以通过指挥飞机通过一个机动序列,比较两个惯性惯性单元的差异来测量。结果可以存储起来,以便使用表查找过程进行后续更正。在较长的时间跨度(分钟和小时)内,惯导系统的漂移误差将在传感器角度输出中引入很大的姿态不确定性,如果不加以纠正,将在被测物体的地球坐标中引入很大的位置不确定性。然而,长期的漂移误差可以通过对已知红外恒星的定期飞行观测来纠正。随着当前一代红外焦平面阵列灵敏度的提高和大面积覆盖,有足够数量的恒星可以方便地在白天和夜间在飞机高度定期观测,从而实现传感器的实时绝对位置校准。利用具有典型机载传感器的角分辨率和灵敏度的传感器,已经获得了机载目标的初步地面测量结果,以便对预期的校准性能进行评估。通过结合使用飞机GPS/INS、传感器INS和特定顺序下的周期性恒星观测的一系列飞行校准程序,预计机载红外传感器的绝对姿态可以被校准到传感器系统瞬时视场的一小部分范围内。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Airborne infrared sensor calibration
Summary form only given, as follows. The employment of sub-milliradian infrared measurement sensors in an airborne platform requires extraordinary techniques to permit the attainment of the parameter accuracy in Earth coordinates vs aircraft coordinates. The airborne platform, in general, contains a GPS/INS system located at the approximate center of gravity. The sensors, in general, are located at the extremities of the aircraft. As a result, static and dynamic (i.e. flexure) errors must be calibrated to permit accurate passive measurements of azimuth and elevation angles to an airborne target. The high frequency, dynamic flexure of the sensor location is usually measured and corrected for by a second INS unit collocated with the sensor. Static offset errors due to aircraft flexure under different aircraft maneuvering conditions can usually be measured by commanding the aircraft through a maneuver sequence and comparing the differences in the two INS units. The results may be stored for subsequent corrections using a table-lookup procedure. Over longer time span (minutes and hours), drift errors of the INS will introduce large attitude uncertainties in the sensor angular output, which if uncorrected, will introduce large positional uncertainities in Earth coordinates of the measured objects. The long term drift errors, however, can be corrected by periodic in-flight observations of known infrared stars. With the improved sensitivities and large areal coverage of the current generation of infrared focal plane arrays, there are sufficient number of stars that could be conveniently observed at periodic intervals at aircraft altitude in both day and night to permit absolute positional calibration of the sensor in real-time. Preliminary ground-based measurements of airborne objects have been obtained with sensors having angular resolution and sensitivity typical of airborne sensors to allow evaluation of the expected calibration performance. By incorporating a sequence of in-flight calibration procedures employing the aircraft GPS/INS, the sensor INS, and periodic star observations under specific sequence, it is expected that the absolute attitude of an airborne IR sensor can be calibrated to within a small part of the instantaneous field of view of the sensor system.<>
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