首页> 外文会议>5th ESA International Conference on Spacecraft Guidance, Navigation and Control Systems Oct 22-25, 2002 Frascati, Italy >ATTITUDE ESTIMATION FROM MAGNETOMETER AND EARTH-ALBEDO-CORRECTED COARSE SUN SENSOR MEASUREMENTS
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ATTITUDE ESTIMATION FROM MAGNETOMETER AND EARTH-ALBEDO-CORRECTED COARSE SUN SENSOR MEASUREMENTS

机译:磁计和地球赤字校正的粗太阳传感器测量的姿态估计

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摘要

A low cost, robust Attitude Determination System with good accuracy for small satellites can be achieved by using a combination of magnetometer and Coarse Sun Sensor. The Coarse Sun Sensor consists of solar cells placed on each of the six outside surfaces of the satellite. The main measurement error of the Coarse Sun Sensor occurs due to the Earth's albedo which can cause an angular deviation of more than 20 degrees. By modelling the albedo and applying state estimation methods for attitude determination the error can be reduced drastically to less than 1 degree, depending on the conditions. In the first part of this paper the development of the albedo model is presented. In the second part the Extended Kalman Filter used for attitude determination is described. The albedo model of the earth is created using existing reflectivity data. Polynomials to describe the albedo light vector received by a satellite in its orbit are derived. The total light vector and the magnetic field vector, taken from the IGRF model, are used by the Kalman Filter.
机译:通过结合使用磁力计和粗太阳传感器,可以实现一种低成本,功能强大,精度高的小型卫星姿态确定系统。粗太阳传感器由放置在卫星六个外表面上的每个太阳能电池组成。粗太阳传感器的主要测量误差是由于地球的反照率而引起的,它可能导致超过20度的角度偏差。通过对反照率进行建模并将状态估计方法应用于姿态确定,根据条件的不同,误差可以大幅度减少到小于1度。在本文的第一部分中,提出了反照率模型的发展。在第二部分中,描述了用于姿态确定的扩展卡尔曼滤波器。地球的反照率模型是使用现有的反射率数据创建的。得出描述卫星在其轨道上接收的反照率光矢量的多项式。卡尔曼滤波器使用从IGRF模型获得的总光矢量和磁场矢量。

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