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41.
The real dynamic thrust measurement system usually tends to be nonlinear due to the complex characteristics of the rig, pipes connection, etc. For a real dynamic measuring system,the nonlinearity must be eliminated by some adequate methods. In this paper, a nonlinear model of dynamic thrust measurement system is established by using radial basis function neural network(RBF-NN), where a novel multi-step force generator is designed to stimulate the nonlinearity of the system, and a practical compensation method for the measurement system using left inverse model is proposed. Left inverse model can be considered as a perfect dynamic compensation of the dynamic thrust measurement system, and in practice, it can be approximated by RBF-NN based on least mean square(LMS) algorithms. Different weights are set for producing the multi-step force, which is the ideal input signal of the nonlinear dynamic thrust measurement system. The validity of the compensation method depends on the engine’s performance and the tolerance error0.5%, which is commonly demanded in engineering. Results from simulations and experiments show that the practical compensation using left inverse model based on RBF-NN in dynamic thrust measuring system can yield high tracking accuracy than the conventional methods. 相似文献
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电容式MEMS角速率传感器零位的全温稳定性是其实用化的最重要的技术指标之一。分析了陀螺工作原理,从传感器敏感表头的空气阻尼、谐振频率等方面分析了机械结构的温度特性,得出了在全温区内驱动力与传感器零位输出的相关性。根据对陀螺表头和接口电路的温度特性分析,设计了恒定跨导高线性度的运算放大器,实现了全温低相位偏移、低幅值偏移的接口ASIC,并在高压N阱COMS工艺下流片。通过驱动力信号对零位进行温度补偿,包含了机械结构刚度和空气热阻尼等因素的影响,理论上比单独的谐振频率补偿更准确,而且驱动力信号可直接由接口电路给出,避免复杂的采样。在-40℃60℃的温度范围内进行零位温度循环测试,驱动力幅值对零位输出进行三阶拟合补偿,补偿后全温零位温度漂移小于26.7(°)/h(1σ)。 相似文献
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基于三自由度飞行动力学模型和运动学模型,提出了一种带有灰色补偿的反步(Back-stepping)控制方法,以实现某些预定的战术机动动作。首先,将飞行动力学模型和运动学模型分解成3个轴方向的相对简单的子系统;然后,针对3个子系统采用反步法分别设计出模型中没有干扰时的控制律,并采用GM(0,N)预测模型对不确定部分的模型参数进行辨识,进一步根据估计出的参数设计灰色补偿控制律;最后,根据3个子系统设计出的控制律解算出同时满足3个子系统渐进稳定的控制输入,这样使得整个系统渐进稳定。仿真结果表明,GM(0,N)预测模型能精确预测不确定模型参数,该算法能够高效实现预定的战术机动动作。 相似文献
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Ali G. Hafez Essam Ghamry Hideki Yayama Kiyohumi Yumoto 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
Geomagnetic storm sudden commencements (SSC) contain a wealth of information which is useful in many applications. It is important to point out that the SSCs used in this study are sampled at the rate of one sample per second in order get use of such high resolution data. In this paper, two studies are made on the geomagnetic SSC and an SSC onset automatic detection algorithm is introduced. The first study is about finding the relationship between the SSC rise time and its amplitude. Where it is found that there is a positive correlation between the amplitude and the amplitude gradient which is the amplitude divided by rise time. The second study is checking the spectrum of the SSC, starting from its onset until the end of the SSC rise time. This check had proved that the SSC contains both low and high frequency regions. This led us to introduce a new term, namely the SSC variation rate (VR). This VR is defined as the maximum rate of change of the field in the higher-frequency region of the SSC. These two studies were the guide to build an SSC automatic detector of one sample per second data using multi resolution analysis (MRA) of the discrete wavelet transform (DWT). The data set contains 134 SSCs with different VRs that were collected from the Circum-pan Pacific Magnetometer Network (CPMN). It is found that the standard deviation of the detection error is 41 s and that the average error is 9 s. From the calculated error distribution function, it is found that the detection error is within the range of −1.5 to 3 min. The detection process, as will be shown in the article, takes 70 s for one station and 3 min if the decision is related to the detection(s) of other stations. These results demonstrate the superiority of the proposed algorithm over other algorithms in which the detection error ranges between −8 and 5 min and the detection process takes 2–10 min. In addition to being faster and more accurate than the other algorithms, the proposed algorithm is the first algorithm that automatically detects the SSC onset times from high-resolution data unlike previous studies that focused on determining the SSC times automatically using one-minute resolution data. 相似文献
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航天器扫描镜成像位置误差补偿技术 总被引:1,自引:0,他引:1
研究地球静止轨道航天器两自由度扫描镜成像位置误差补偿问题,即通过对扫描角的补偿,使光轴在地球表面的成像点位置与标称位置相同,消除探测区域的位置偏差.在考虑扫描镜法线偏移、姿态偏差以及轨道误差条件下,推导了光轴成像点的地心经纬度计算公式.给出了上述3类误差的具体描述方式,并分析了各种误差对光轴成像点位置的影响关系.基于角度误差的小量假设条件,给出了扫描镜的步进角/扫描角补偿量的显式算法.针对法线偏移信息一般难以准确测量的问题,提出了一种利用扫描镜在特定工作模式下的光轴惯性空间定向能力和法线偏移的长周期特性对其进行估计的方法.仿真结果表明,所提出的补偿方案和算法能够显著提高成像点位置精度. 相似文献
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