分岔参数的分维数识别法

广泛用于各行各业的转子系统的稳定性问题一直倍受关注。而在当今失稳多是由于一些非线性现象的出现所引起,这就对转子系统的设计提出了更高的要求：考虑非线性因素,避开会出现非线性现象的不稳定参数点或区域。本文中通过对一经典倍周期分岔模型—Ｍａｙ 模型及单盘Ｊｅｆｆｃｏｔｔ转子的研究,得出了利用随参数变化的时间序列分维数趋势图,可以很好地识别非线性动力系统发生分岔时的临界参数     

A priori zenith wet delays in the analysis of VLBI CONT sessions

Tropospheric delay is one of the major sources of error in VLBI (Very Long Baseline Interferometry) analysis. The principal component of this error can be accurately computed through reliable surface pressure data —hydrostatic delay— yet there is also a small but volatile component —wet delay— which is difficult to be modelled a priori. In VLBI analysis, troposphere delay is typically modelled in the theoretical delays using Zenith Hydrostatic Delays (ZHD) and a dry mapping function. Zenith Wet Delay (ZWD) is not modelled but estimated in the analysis process. This work studies inter alia the impact of including external GNSS estimates to model a priori ZWD in VLBI analysis, as well as other models of a priori ZWD.In a first stage, two different sources of GNSS troposphere products are compared to VLBI troposphere estimates in a period of 5 years. The solution with the best agreement to VLBI results is injected in the VLBI analysis as a priori ZWD value and is compared to other options to model a priori ZWD. The dataset used for this empirical analysis consists of the six CONT campaigns.It has been found that modelling a priori ZWD has no significant impact either on baseline length and coordinates repeatabilities. Nevertheless, modelling a priori ZWD can change the magnitude of the estimated coordinates a few millimeters in the up component with respect to the non-modelling approach. In addition, the influence of a priori ZWD on Earth Orientation Parameters (EOP) and troposphere estimates —Zenith Total Delays (ZTD) and gradients—has also been analysed, resulting in a small but significant impact on both geodetic products.     

轨道测量差分精确定轨方法

航天器轨道精确测定重要环节之一是有效地消除观测系统误差,在轨道测量数据处理时,一类是利用轨道约束自校准技术来估算和校准系统误差,另一类可以应用测元差分方法来消除系统误差(例如导航卫星测定目标)。本文提出一种新的差分技术,即利用观测数据时序差分消除系统误差技术,并推导相应确定航天器轨道的公式。     

应用变速控制力矩陀螺的卫星姿态机动的非线性控制

研究了以变速控制力矩陀螺(VSCMG)作为执行机构的卫星多目标快速机动的控制问题。首先建立了带有多个变速控制力矩陀螺的航天器姿态动力学模型,采用修正的罗德里格斯参数(MRP)描述姿态运动。在考虑执行机构饱和、机动速率限制、控制带宽限制等情况下,设计了基于Lyapunov理论的非线性姿态反馈控制器。针对外部干扰会使控制力矩陀螺的框架角偏移其标称值的情况,采取磁补偿控制来保持框架角在一定范围变化。以采用VSCMG为执行机构的某卫星为例进行了数值仿真,仿真结果验证了提出的非线性姿态反馈控制器的有效性,采取的磁补偿控制也很好地抑制了变速控制力矩陀螺框架角的偏移。     

低压涡轮气动/声学一体化设计——总体参数优化

低压涡轮是航空发动机的重要噪声源之一,同时也是影响发动机单位推力耗油率的重要部件之一。为适应新一代发动机高效、低噪的设计目标,提出了基于传统涡轮设计流程的低压涡轮气动/声学一体化设计思路,并以某一典型民用发动机6级低压涡轮的设计要求为例,对末级功分配、通道外径、涡轮出口马赫数、叶片数目等涡轮总体参数进行了优化探索。结果表明,文中提出的设计思路可以在涡轮设计的总体参数选取阶段对涡轮效率和噪声同时进行有效评估,以便合理地选取涡轮总体参数,是一种可行的高效、低噪涡轮设计方法。     

航空发动机仿真模型参数自适应校正

采用修正因子方法建立自适应仿真模型,运用改进的共轭梯度算法求解非线性规划问题,依据发动机台架试车和空中试飞测量数据,对发动机仿真模型的部件特性参数进行校正,使模型的计算输出与试验测量数据吻合。应用本文方法对某型双转子加力涡喷发动机仿真模型进行校正,获得了满意的仿真精度。     

ITRS/GCRS transformation: Uncertainty propagation analysis and short-term modelling of IAU 2006/2000A developments

A study of the uncertainty propagation in ITRS/GCRS transformation is presented in this work. General law of propagation of variances is applied to the ITRS/GCRS transformation matrix, deriving the analytical expressions to compute GCRS position uncertainty. This evaluation is based on EOP uncertainties provided by IERS long-term series and formal uncertainties of ITRS-compatible coordinates. Numerical results for the period 1998–2016 are shown and discussed for ITRS positions in different altitudes and latitudes, providing graphical and numerical insights of the mapping of EOP uncertainties to transformed coordinates.Eventually, an analysis of short-term evolution of the Celestial Intermediate Pole coordinates in the GCRS provided by the IAU2006/2000A precession-nutation model is carried out, in order to assess the feasibility to potentially broadcast these parameters in GNSS navigation message. This approach would facilitate the dissemination of terrestrial-celestial transformation parameters for real time users, given that polar motion and UT1-UTC are already foreseen in GPS interface specification. The results presented in this work confirm the feasibility of this idea.     

无陀螺下基于修正罗德里格参数的星体姿态确定

介绍了修正罗德里格参数(MRP),分析比较了姿态表示参数修正罗德里格参数和四元数的算法特点。通过仿真计算,比较了当卫星受一阶马尔柯夫干扰力矩作用和CCD星敏感器为唯一星载角运动传感器时,分别用修正罗德里格参数和四元数作为姿态表示参数,采用UKF(Unscented Kalman Filter)估计卫星航向、姿态及相应角速率的滤波效果。结果表明,用修正罗德里格参数法的姿态解算精度比用四元数法的姿态解算精度高,且计算效率明显优于四元数算法,计算量仅相当于四元数算法的一半,这是由于四元数的规范化条件(即模值为1),在姿态确定中会导致误差协方差阵奇异,而修正罗德里格参数虽然不是全局非奇异的,但是可以通过切换方法解决奇异性问题。     

变PID参数控制在电动齿轮燃油泵中的应用CSCD

为实现电动齿轮燃油泵系统的精确供油控制,建立了电动齿轮燃油泵流量特性模型,设计了数字式PID参数控制,并在此基础上以参数切换为原则设计了变PID参数控制,以满足不同情况下航空发动机对供油量的需求。通过试验,变参数PID控制实现了对电动齿轮燃油泵的精确控制,说明设计的PID控制规律能够应用于电动齿轮燃油泵系统供油量的闭环控制。     

参考系选择对Kepler广播星历参数拟合精度的影响

通过对MEO、IGSO、GEO三类导航卫星广播星历的开普勒轨道根数拟合方法及其拟合精度的分析研究,得出结论:开普勒轨道根数拟合导航卫星广播星历的方法,能很好吸收坐标变换过程中岁差、章动、极移、地球自转等因素对卫星星历拟合精度的影响。