捕获轨迹系统并联机构地面标定方法

捕获轨迹系统（CTS）是一种先进的预测外挂物投放轨迹的试验系统，普遍采用六自由度（6-DoF）串联机构作为其运动机构，串联机构因惯性力大和关节累积误差大使其定位精准度不足。相比串联机构，并联机构具有惯性力小和关节误差不累积等优点。采用6-PTRT并联机构作为CTS试验系统的六自由度运动机构，在空间受限的风洞环境中对CTS并联机构进行地面标定：提出动平台位姿的测量和计算方法，建立包含直线驱动平台安装夹角修正的标定模型，并基于非线性最小二乘法辨识结构参数。辨识后CTS并联机构的位移定位准度优于0.1 mm，姿态定位准度优于0.05°，最后以CTS并联机构和常规攻角机构进行8#标模的对比风洞试验。风洞试验结果表明，CTS并联机构的风载定位准度满足测力试验精准度要求。     

飞机活动半径与飞行等时点

飞机活动半径与飞行等时点是在特殊或者紧急飞行情况下,根据飞机实际油量选定最有利的紧急备降机场,保证飞机在安全距离或者最短时间内在备降机场降落的一种紧急情况处置方法。本文通过理论分析和实例验证,提出在曲折航线飞行中,用实际飞行资料精确计算飞机活动半径和飞行等时点位置的新的计算方法。     

一种二自由度球形五杆并联机构的运动学分析

应用螺旋理论分析一种二自由度球形五杆并联机构的运动螺旋及其反螺旋，在此基础上分析了其自由度。建立其位置正、反解方程，并进行验证。应用螺旋理论建立了其一阶影响系数矩阵。     

电位法测量微缺口试样的数值分析

疲劳寿命受到材料内部缺陷的制约,可以通过电位法试验获得微缺口试样的疲劳裂纹扩展规律,进而分析缺陷对材料疲劳寿命的影响。在试验前,需要预先研究试验的主要影响因素。利用COMSOL有限元软件,研究了电流输入点位置和电势差测点位置对试验精度和试验复现性的影响,计算得到不同裂纹前缘形状对应的电位法校核曲线。结果表明:(1)电流输入点位置位于试样平行于裂纹面的上下表面时,可以保证试验的复现性。(2)当测点位于裂纹面的垂直对称面上,且测点距离裂纹面垂直距离为0.06～0.1倍试样宽度时,可以同时满足测试精度和复现性。(3)当裂纹宽度和裂纹深度的比值3时,可以不考虑裂纹前缘形状对校核曲线的影响,当裂纹宽度和裂纹深度的比值≤3时,裂纹前缘形状对校核曲线的影响较大。     

低雷诺数下双元素翼帆的襟翼几何参数对其推进特性影响研究

为了研究大型船舶在航行中翼帆对其推进性能的影响规律,本文建立了一种双元素翼帆模型,并采用雷诺平均N-S方程在定常和非定常工况下对襟翼几何参数变化的模型进行数值仿真。结果表明,双元素翼帆气动特性的改变体现了襟翼旋转轴位置、襟翼偏转角以及缝隙宽度之间的非线性耦合作用。襟翼旋转轴位置的前移实际上是增大了缝隙宽度,进而增加了流过缝隙的流体,避免了主翼尾流的流动分离。然而,襟翼旋转轴位置的前移距离也受到襟翼偏转角的限制,在襟翼偏转角为25°、攻角为6°,当襟翼旋转轴位置由90%前移到85%时,襟翼吸力面发生了大尺度流动分离。襟翼旋转轴位置不宜过于靠前或靠后,当相对缝隙宽度为2.4%时襟翼旋转轴位置为85%较为合理。     

An approach for parameter estimation of combined CPPM and LFM radar signal

In this paper, the problem of parameter estimation of the combined radar signal adopting chaotic pulse position modulation (CPPM) and linear frequency modulation (LFM), which can be widely used in electronic countermeasures, is addressed. An approach is proposed to estimate the initial frequency and chirp rate of the combined signal by exploiting the second-order cyclostationarity of the intra-pulse signal. In addition, under the condition of the equal pulse width, the pulse repetition interval (PRI) of the combined signal is predicted using the low-order Volterra adaptive filter. Simulations demonstrate that the proposed cyclic autocorrelation Hough transform (CHT) algorithm is theoretically tolerant to additive white Gaussian noise. When the value of signal noise to ratio (SNR) is less than 4 dB, it can still estimate the intra-pulse parameters well. When SNR = 3 dB, a good prediction of the PRI sequence can be achieved by the Volterra adaptive filter algorithm, even only 100 training samples.     

Research on uncertainty in measurement assisted alignment in aircraft assembly

Operations in assembling and joining large size aircraft components are changed to novel digital and flexible ways by digital measurement assisted alignment.Positions and orientations（P＆O）of aligned components are critical characters which assure geometrical positions and relationships of those components.Therefore,evaluating the P＆O of a component is considered necessary and critical for ensuring accuracy in aircraft assembly.Uncertainty of position and orientation（U-P＆O）,as a part of the evaluating result of P＆O,needs to be given for ensuring the integrity and credibility of the result;furthermore,U-P＆O is necessary for error tracing and quality evaluating of measurement assisted aircraft assembly.However,current research mainly focuses on the process integration of measurement with assembly,and usually ignores the uncertainty of measured result and its influence on quality evaluation.This paper focuses on the expression,analysis,and application of U-P＆O in measurement assisted alignment.The geometrical and algebraical connotations of U-P＆O are presented.Then,an analytical algorithm for evaluating the multi-dimensional U-P＆O is given,and the effect factors and characteristics of U-P＆O are discussed.Finally,U-P＆O is used to evaluate alignment in aircraft assembly for quality evaluating and improving.Cases are introduced with the methodology.     

Explicit expression of collision probability in terms of RSW and NTW components of relative position

The existing analytical and numerical computing methods for collision probability (P_c) provide sufficiently accurate results, but do not reveal the direct connection between P_c and conjunction geometry or error covariance. This paper derived an explicit expression of P_c under the circular orbit assumption, based on analysis of closest approach distance and Chan’s analytical formulae for P_c. The P_c was expressed as an explicit function of the radial, in-track, cross-track components of relative position and error covariance. The explicit expression is simple and compact, relates P_c with components of relative position, which are two kinds of important conjunction risk criteria. By introducing non-zero flight-path angle and ratio of velocity’s magnitude, a modified expression of P_c was presented for objects in eccentric orbits. For objects with eccentricity less than 0.01 (which account for 62% of all LEO objects), the relative error of the explicit expression is less than 0.107, or 0.252 for typical conjunction cases. What really matters in conjunction risk assessment is the order of magnitude rather than the specific value of P_c, the precision of the explicit expression is sufficient for conjunction risk assessment and decision-making for most LEO objects.     

改进的卫星广播星历参数模型及其算法

考虑导航卫星受地球周期性的摄动力影响,提出了一种改进的导航卫星星历参数模型,给出了模型参数的计算方法和用该模型外推卫星轨道的计算步骤。仿真计算结果表明：该广播星历参数模型外推能力强,可较好地拟合卫星运动轨道。     

Formation control using μ-synthesis for Inner-Formation Gravity Measurement Satellite System

Inner-Formation Gravity Measurement Satellite System (IFGMSS) is used to map the gravity field of Earth. The IFGMSS consists of two satellites in which one is called “inner satellite” and the other one is named as “outer satellite”. To measure the pure Earth gravity, the inner satellite is located in the cavity of the outer satellite. Because of the shield effect of the cavity, the inner satellite is affected only by the gravitational force, so it can sense Earth gravity precisely. To avoid the collision between the inner satellite and the outer satellite, it is best to perform a real-time control on the outer satellite. In orbit, the mass of the outer satellite decreases with the consumption of its propellant. The orbit angular rate of the inner satellite varies with time due to various disturbing forces. These two parameters’ uncertainties make the C–W function be not so accurate to describe the formation behavior of these two satellites. Furthermore, the thrusters also have some uncertainties due to the unmodelled dynamics. To cancel the effects caused by the above uncertainties, we have studied the robust control method based on the μ-synthesis. This μ-synthesis eliminates the conservativeness and improves the control efficiency comparing with the H_∞ method. Finally, to test the control method, we simulate an IFGMSS mission in which the satellite runs in a sun synchronous circular orbit with an altitude of 300 km. The simulation results show the effectiveness of the robust control method. The performances of the closed-loop system with the μ-controller are tested by the μ-analysis. It has found that the nominal performance, the robust stability and the robust performance are all achieved. The transient simulation results further prove the control response is fast and the accuracy of the relative position meets the demand of the gravity measurement.