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A Novel Multi-Aperture Based Sun Sensor Based on a Fast Multi-Point MEANSHIFT (FMMS) Algorithm

机译:基于快速多点MEANSHIFT(FMMS)算法的基于多孔径的新型太阳传感器

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With the current increased widespread interest in the development and applications of microanosatellites, it was found that we needed to design a small high accuracy satellite attitude determination system, because the star trackers widely used in large satellites are large and heavy, and therefore not suitable for installation on microanosatellites. A Sun sensor + magnetometer is proven to be a better alternative, but the conventional sun sensor has low accuracy, and cannot meet the requirements of the attitude determination systems of microanosatellites, so the development of a small high accuracy sun sensor with high reliability is very significant. This paper presents a multi-aperture based sun sensor, which is composed of a micro-electro-mechanical system (MEMS) mask with 36 apertures and an active pixels sensor (APS) CMOS placed below the mask at a certain distance. A novel fast multi-point MEANSHIFT (FMMS) algorithm is proposed to improve the accuracy and reliability, the two key performance features, of an APS sun sensor. When the sunlight illuminates the sensor, a sun spot array image is formed on the APS detector. Then the sun angles can be derived by analyzing the aperture image location on the detector via the FMMS algorithm. With this system, the centroid accuracy of the sun image can reach 0.01 pixels, without increasing the weight and power consumption, even when some missing apertures and bad pixels appear on the detector due to aging of the devices and operation in a harsh space environment, while the pointing accuracy of the single-aperture sun sensor using the conventional correlation algorithm is only 0.05 pixels.
机译:随着当前对微型/纳米卫星的开发和应用的广泛兴趣,我们发现我们需要设计一种小型高精度卫星姿态确定系统,因为广泛用于大型卫星的恒星跟踪器又大又重,因此适用于安装在微型/纳米卫星上。事实证明,太阳传感器+磁力计是更好的选择,但是传统的太阳传感器精度低,无法满足微/纳卫星姿态确定系统的要求,因此开发了一种具有高可靠性的小型高精度太阳传感器非常重要本文提出了一种基于多孔径的阳光传感器,该传感器由一个具有36个孔的微机电系统(MEMS)掩模和一个位于该掩模下方一定距离的有源像素传感器(APS)CMOS组成。提出了一种新颖的快速多点MEANSHIFT(FMMS)算法,以提高APS太阳传感器的两个关键性能特征-准确性和可靠性。当阳光照射传感器时,APS检测器上会形成一个太阳斑阵列图像。然后可以通过FMMS算法分析检测器上的光圈图像位置来得出太阳角。使用该系统,即使由于设备的老化和在恶劣的太空环境中的操作而在检测器上出现一些缺失的光圈和不良像素,太阳图像的质心精度也可以达到0.01像素,而不会增加重量和功耗。而采用常规相关算法的单孔太阳传感器的指向精度仅为0.05像素。

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