费率受制于位相半马氏过程的风险模型

对带马氏链的线性和非线性系统，经过众多学者近20多年的努力，已取得一系列重要成果。然而，由于马氏链状态逗留时间服从负指数分布，使得这些成果在应用中有很大的局限性。本文首先探讨了位相半马氏过程的性质，然后以位相半马氏过程代替马氏过程，研究风险模型的相关问题，取得了与马氏链相同的研究成果，从而说明了位相半马氏过程在克服由马氏过程带来的局限性中的作用。     

Wind asymmetries in massive stars

We are in the process of surveying the linear polarization in luminous, early-type stars. We here report on new observations of the B [e] stars S 18 and R 50, and of the Luminous Blue Variables HR Car, R 143, and HD 160529. Together with previously published data, these observations provide clear evidence for the presence of intrinsic polarization in 1 B[e] star (HD 34664) and in 5 LBVs ( Car, P Cyg, R 127, AG Car, and HR Car). The data indicate that anisotropic stellar winds are a common occurrence among massive stars in these particular evolutionary stages. For such stars, mass-loss rates estimated using the assumption of a spherical, homogeneous and stationary outflow may be in error.     

确定微动疲劳寿命的附加应力法

通过引进新的微动疲劳参数 ,对微动疲劳寿命进行定量分析。将微动作用的效果作为一种附加应力 ,与普通力学分析中得到的宏观应力一起作为总应力作用于构件。用这个总应力按疲劳寿命计算公式或对照疲劳寿命S -N曲线得到疲劳寿命 ,这个疲劳寿命就是微动疲劳寿命。这种方法称为附加应力法。     

静载下含平面缺陷的压力管道的失效率

参照 SAPV-95规范,用第 2水平法对静载下含平面缺陷的压力管道进行了可靠性分析,得出了功能函数。提出了计算失效率的快速收敛的迭代算法,并分析了失效率与广义强度和广义应力的均值及变异系数的关系。得出了用失效率可对静载下含平面缺陷的压力管道的安全状况进行评估和预测的结论     

雷达天线罩廓形误差评定研究

 就弹载或飞行器上雷达天线罩的廓形测量及测量精度提高,探讨了应用鞍点规划的方法对天线罩廓形误差进行评定,给出了评定的线性鞍点规划模型,评定的最小条件,以及具体的操作处理方法,并介绍了评估例子,表明应用本文的评定方法获得了良好的结果。     

无人直升机的动态逆模糊集成控制

对于一个非线性系统,利用其近似的线性化模型求出系统的近似逆,采用模糊控制方法抑制误差对系统输出的影响来保证系统的最终特性,构成一种动态逆模糊集成控制方案.将这一方法应用在无人直升机的姿态控制中,仿真结果表明该方法可以消除无人机未建模动态和不确定性的影响,具有较好的鲁棒性能.      

约化代数自伴的充要条件

约化代数是自伴的吗?这是一个知名的问题,至今没有解决。它的肯定的回答将蕴含可传代数问题及约化算子问题的肯定回答。在这篇文章中,我们找到了约化代数是自伴的几个充要条件。例如,我们得到:约化代数u是自伴的充要条件是对于每个n≥2,u~(n)的每个稠定义的不变图形子空间是约化子空间。     

The adjusted optical properties for Galileo/BeiDou-2/QZS-1 satellites and initial results on BeiDou-3e and QZS-2 satellites

Solar Radiation Pressure (SRP) is the dominant non-gravitational perturbation for GNSS (Global Navigation Satellite System) satellites. In the absence of precise surface models, the Empirical CODE Orbit Models (ECOM, ECOM2) are widely used in GNSS satellite orbit determination. Based on previous studies, the use of an a priori box-wing model enhances the ECOM model, especially if the spacecraft is a stretched body satellite. However, so far not all the GNSS system providers have published their metadata. To ensure a precise use of the a priori box-wing model, we estimate the optical parameters of all the Galileo, BeiDou-2, and QZS-1 (Quasi Zenith Satellite System) satellites based on the physical processes from SRP to acceleration. Validation using orbit prediction proves that the adjusted parameters of Galileo and QZS-1 satellites exhibit almost the same performance as the corresponding published and “best guess” values. Whereas, the estimated parameters of BeiDou-2 satellites demonstrate an improvement of more than 60% over the initial “guess” values. The resulting optical parameters of all the satellites are introduced into an a priori box-wing model, which is jointly used with ECOM and ECOM2 model in the orbit determination. Results show that the pure ECOM2 model exhibits better performance than the pure ECOM model for Galileo, BeiDou-2 GEO and QZS-1 orbits. Combined with the a priori box-wing model the ECOM model (ECOM+BW) results in the best Galileo, BeiDou-2 GEO and QZS-1 orbits. The standard deviation (STD) of satellite laser ranging residuals reduce by about 20% and 5% with respect to the pure ECOM2 model for Galileo and BeiDou-2 GEO orbits, while the reductions are about 40% and 60% for QZS-1 orbits in yaw-steering and orbit-normal mode respectively. BeiDou-2 IGSO and MEO satellite orbits do not benefit much from the a priori box-wing model. In summary, we suggest setting up a unified SRP model of ECOM+BW for Galileo, QZS-1, and BeiDou-2 orbits based on the adjusted metadata. In addition, we estimate the optical parameters of BeiDou-3e and QZS-2 satellites using a limited number of tracking stations. Results regarding the unified SRP model indicate the same advantages, the STD of satellite laser ranging residuals reduces by about 30% and 20% for QZS-2 and BeiDou-3e orbits respectively over orbit products without a priori model. The estimation procedure is effective and easy to apply to the new emerging satellites in the future.     

嫦娥三号探测器连续姿控的轨道动力学模型补偿及实现

针对嫦娥三号探测器的连续姿控喷气对飞行轨道产生的扰动影响,在精密定轨中建立了经验力补偿模型,并使用最小二乘估计算法计算经验力模型参数与探测器轨道。通过重叠弧段轨道精度评估法对该模型补偿效果进行了验证,结果显示,定轨预报的星历误差以及拟合残差均有所改善,特别是环月轨道的定轨精度由百米量级提高到十米量级。     

Robust Hybrid Control for Ballistic Missile Longitudinal Autopilot

This paper investigates the boost phase’s longitudinal autopilot of a ballistic missile equipped with thrust vector control. The existing longitudinal autopilot employs time-invariant passive resistor-inductor-capacitor (RLC) network compensator as a control strategy, which does not take into account the time-varying missile dynamics. This may cause the closed-loop system instability in the presence of large disturbance and dynamics uncertainty. Therefore, the existing controller should be redesigned to achieve more stable vehicle response. In this paper, based on gain-scheduling adaptive control strategy, two different types of optimal controllers are proposed. The first controller is gain-scheduled optimal tuning-proportional-integral-derivative (PID) with actuator constraints, which supplies better response but requires a priori knowledge of the system dynamics. Moreover, the controller has oscillatory response in the presence of dynamic uncertainty. Taking this into account, gain-scheduled optimal linear quadratic (LQ) in conjunction with optimal tuning-compensator offers the greatest scope for controller improvement in the presence of dynamic uncertainty and large disturbance. The latter controller is tested through various scenarios for the validated nonlinear dynamic flight model of the real ballistic missile system with autopilot exposed to external disturbances.