分数阶不确定混沌系统鲁棒投影同步控制

基于滑模变结构控制理论,选取了一种分数阶滑模面,针对分数阶系统不确定项上界已知情况,提出了一种鲁棒控制方法,将这种控制方法与范数不等式相结合对系统的稳定性进行了分析。该控制器能够很好地抑制不确定因素对误差系统的影响,能够快速实现驱动系统与响应系统的同步。最后,将该鲁棒控制策略应用于分数阶混沌系统数字保密通信中,数值仿真验证了该方案的正确性和有效性。     

润滑油红外光谱去噪预处理方法

采用小波包变换软阈值去噪方法对润滑油的红外光谱进行去噪预处理,结合偏最小二乘法进行定量预测,并与常用的平滑去噪方法进行对比。结果表明,小波包变换能有效地去除红外光谱的噪声,以此为基础建立的润滑油酸值模型的预测精度高于常用的平均平滑法和 Savitzky-Golay卷积平滑法这 2种平滑去噪方法的预测精度。     

Cramér-rao lower bound for pulsar rotation parameters estimation with X-ray pulsar observation data

In this paper, the Cramér-Rao Lower Bound (CRLB) for estimating the rotation parameters of pulsars using X-ray pulsar observation data is deduced, and the calculation equation is presented. In order to verify the correctness of the deduced equation, we use the X-ray pulsar observation data to estimate pulsar rotation parameters, and obtain the root mean square error (RMSE) of the estimated pulsar rotation parameters through conducting repeated experiments. The experimental results suggest that when the observation time increases, the RMSE gradually approaches the estimated CRLB, and that when the observation time is 2.4 × 10⁶ s, the error between the RMSE of pulsar frequency estimation and the CRLB stays at 10^?11 order of magnitude. This verifies that the CRLB expression deduced in this paper is the theoretical lower bound for estimating pulsar rotation parameters. The deduced CRLB in this paper helps determine the minimum variance estimator for pulsar rotation parameter estimation using X-ray pulsar data, providing a benchmark for the comparison between the minimum variance estimator and other estimators.