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EFFECTS OF INCLINOMETER ERROR ON STAR SENSOR POSITION ACCURACY

机译:倾斜度误差对恒星传感器位置精度的影响

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Recently attempts to find a solution to compensate for Global Positioning System (GPS) deficiencies has increased due to various requirements from civil and military applications. These deficiencies include mainly intentional or unintentional loss or manipulation of signals which leads to loss of precise position information. Several replacements for GPS have been introduced so far but one of the potential candidates is utilization of star sensors. For position determination using star tracker the information of orientation, exact time of capturing the star image and deviation from local vertical arc required. Orientation is determined by default application of available star sensors. Image capturing time can be provided from onboard timing systems which can vary from GPS to atomic clock. Deviation from local vertical can be determined using a set of inclinometers or Inertial Measurement Unit including gyroscope. Accuracy of resulting system depends on these three main elements as well. Bright point position which effects the accuracy of transfer matrix between Inertial and Body reference frame. Time accuracy effects the transfer matrix between Greenwich and Inertial reference frame. Accuracy of inclinometer effects transfer matrix between local horizontal plane and Body frame which has an important role on overall position determination accuracy. In this paper effect of inclination measurement accuracy on position results are analyzed using Monte-Carlo simulation. For this purpose 200 random positions arc simulated. Camera boresight in each position is pointed to sky in equal steps between -30 to +30 degree zenith angle. The only source of error is placed on inclinometer accuracy in measuring the stable platform inclination from horizon. In each position 1000 images with random error on inclinometer arc examined. No additional error such as bright point position or time is applied to examine the nominal performance of position determination. Using sequential transfer matrix method, attitude matrix along with timing information and transfer matrix between local horizontal plane and body frame arc combined to derive the same position that is initially simulated. Results demonstrate that position determination using star tracker shows its highest accuracy while aligned in the opposite direction of local vertical or zenith. Net error increases while deviating from zenith depending on inclinometer resolution. This study demonstrates that 0.001 degree nominal accuracy is acceptable within aforementioned range of zenith deflection. Therefore depending on hardware overall precision, more common inclinometers can be selected to reduce the fixed price.
机译:最近,由于民用和军用的各种要求,寻找弥补全球定位系统(GPS)缺陷的解决方案的尝试已经增多。这些缺陷主要包括有意或无意的丢失或对信号的操纵,这导致丢失精确的位置信息。到目前为止,已经引入了GPS的几种替代品,但潜在的候选者之一是利用星型传感器。对于使用星形跟踪器确定位置的信息,包括方向信息,捕获星形图像的准确时间以及与局部垂直弧的偏差。方向由可用恒星传感器的默认应用程序确定。可以从车载定时系统提供图像捕获时间,该定时系统可以从GPS到原子钟变化。可以使用一组倾斜仪或惯性测量单元(包括陀螺仪)来确定与局部垂直方向的偏差。最终系统的准确性也取决于这三个主要因素。亮点位置会影响惯性和身体参考系之间传递矩阵的准确性。时间精度会影响格林威治和惯性参考系之间的传递矩阵。测斜仪的精度会影响局部水平面与车身框架之间的传递矩阵,这对整体位置确定精度具有重要作用。在本文中,使用蒙特卡洛模拟分析了倾斜度测量精度对位置结果的影响。为此,模拟了200个随机位置。每个位置的摄像机视轴都以-30至+30度的天顶角等距指向天空。误差的唯一来源是测斜仪的精度,以测量从地平线到平台的稳定倾斜度。在每个位置检查了1000张在倾斜仪上具有随机误差的图像。不会应用诸如亮点位置或时间之类的其他错误来检查位置确定的标称性能。使用顺序转移矩阵方法,将姿态矩阵与时间信息以及局部水平面和车身框架之间的转移矩阵结合起来,得出最初模拟的相同位置。结果表明,使用恒星跟踪仪进行位置确定时,在与局部垂直方向或天顶方向相反的方向上对齐时,其精度最高。取决于倾角仪的分辨率,在偏离天顶时,净误差会增加。这项研究表明,在上述天顶挠度范围内,0.001度的标称精度是可以接受的。因此,根据硬件的整体精度,可以选择更常见的测斜仪以降低固定价格。

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