首页> 外文会议>58th International Astronautical Congress 2007 >SATELLITE ACTIVE MAGNETIC ATTITUDE CONTROL SYSTEM IN SAFE HOLD MODE
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SATELLITE ACTIVE MAGNETIC ATTITUDE CONTROL SYSTEM IN SAFE HOLD MODE

机译:安全保持模式下的卫星有源磁态控制系统

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Explored here is the active magnetic attitude control system of a satellite on a polar orbit in the safe hold mode(SHM). Usually, the satellite stays in Normal Mode, An alarm or a ground request could involve a mode exit towards the Safe Hold Mode. In this mode, in order to simplify the hardware of the attitude control system(ACS), thrusters and sophisticated equipment (for instance gyros) are not used. Coarse sun sensors(CSS) and three-axis magnetometers(TAM) provide attitude measurement, and magnetic torquers generate torque. This mode consists in 2 main phases: rate damping phase (RDP), sun pointing phase (SPP). The aim of this mode consists in reaching autonomously a safe attitude with the -Ys satellite axis pointed to the Sun and with the mean three-axis angular rate equal to -0.2 deg/s. When the angular rates are not measured directly, they can be estimated from knowledge of the quaternion vector or the direction cosine matrix, which are obtained from attitude position measurements. Based on a recently introduced method for angular rate estimation of a geostationary satellite from sun direction observations, a new method is presented for estimation of the angular rate in this paper. The estimator consists of an Unscented Kalman Filter(UKF). First, a deterministic algorithm generates a coarse estimate of the satellite angular rate from the sun vector measurements and the readings of a three-axis magnetometer. This rate then used to initialize an Unscented Kalman Filter, thus rendering the resulting estimate highly accurate and robust. Then the controllers of rate damping phase and sun pointing phase are designed. The Regulators are Minus-Dot-B and PID control respectively. Stability and control analysis are presented. Finally, a close-loop simulation is done. Detailed simulation results are presented to demonstrate the performance of the algorithm. This paper has shown that the designed system can meet the technology demand of the safe hold mode.
机译:这里探讨的是处于安全保持模式(SHM)的极地轨道上的卫星的主动磁姿态控制系统。通常,卫星处于正常模式,警报或地面请求可能会导致模式退出而进入安全保持模式。在这种模式下,为了简化姿态控制系统(ACS)的硬件,不使用推进器和复杂的设备(例如陀螺仪)。粗大的太阳传感器(CSS)和三轴磁力计(TAM)提供姿态测量,而磁性扭矩产生扭矩。此模式包含2个主要阶段:速率衰减阶段(RDP),阳光指向阶段(SPP)。该模式的目的在于使-Ys卫星轴指向太阳,并且三轴平均角速度等于-0.2度/秒,从而自动达到安全姿态。当不直接测量角速度时,可以根据四元数向量或方向余弦矩阵的知识来估算角速度,这些四元数向量或方向余弦矩阵是从姿态位置测量中获得的。基于最近介绍的一种基于太阳方向观测的对地静止卫星角速率估计方法,提出了一种估计角速率的新方法。估计器由无味卡尔曼滤波器(UKF)组成。首先,确定性算法根据太阳矢量测量值和三轴磁力计的读数生成卫星角速率的粗略估计。然后,该速率用于初始化无味卡尔曼滤波器,从而使结果估算高度准确且稳健。然后设计了速率衰减阶段和太阳指向阶段的控制器。调节器分别为负点B和PID控制。介绍了稳定性和控制分析。最后,完成了闭环仿真。给出了详细的仿真结果以证明该算法的性能。本文表明,所设计的系统可以满足安全保持模式的技术要求。

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