基于磁导率法的零部件硬度电磁无损检测技术研究

传统的机械压痕法虽能测量火炮零部件的硬度,但对其表面有损害,且某些零部件工作面并不允许使用打点测量方式．为解决这一问题,基于硬度与材料磁导率之间的对应关系,设计了一种硬度电磁无损检测系统,采用DDS技术实现参数可控的正弦信号源,以满足磁导率测试所需的激励条件．为了提高检测灵敏度,利用交流电桥拾取由硬度变化引起的检测线圈和参考线圈电压差分信号,并进一步在调理电路中采用正交锁相放大技术对这一微弱信号进行放大和噪声抑制．硬度试验结果表明,该系统能以无损的检测方式有效地区分零部件的硬度值,为火炮定型试验中的硬度测量提供了新途径．     

静止条件下多种轨道-电枢形状的轨道炮电流分布仿真

针对等轨道截面、等炮口截面、等长度、等材料和等电流8种典型的轨道-电枢结构,在电枢速度为0 m／s的情况下,采用Ansoftl 2有限元分析软件,仿真分析电流分布特征,得到：矩形截面轨道一长方体结构电枢的轨道炮有最不均匀的电流分布特征,电流主要分布在轨道外表面和电枢后部凹表面,并且分别对应于趋肤效应和电流短路径聚集现象,跑道形截面的轨道一回转体结构电枢的轨道炮有最均匀的电流密度分布．     

复合陶瓷含片状夹杂共晶体的理论断裂强度

应用四相模型法研究含片状夹杂复合共晶体的细观应力场．在基体、界面相和片状夹杂为各向同性的条件下,得到细观应力分布规律,并表现出明显的尺度效应．应用位错塞积理论研究片状夹杂内的位错运动,通过两相界面处位错塞积产生的应力集中确定其在基体内产生的最大张应力,导致基体首先被破坏失效,当基体内最大张应力等于分子理论的断裂强度时,得到共晶体断裂强度的理论表达式．结果表明：含片状夹杂共晶复合陶瓷强度随夹杂厚度增加而减小．     

翼栅绕流流场数值模拟及动力性能研究

基于2D不可压缩定常流动的控制方程,对5个NACA4412非对称翼型组成的平面直列翼栅绕流流场进行了数值模拟,对比分析了同一翼型在翼栅中工作和单独绕流时的升、阻力情况,验证了翼栅装置工作的可行性,反映了翼栅绕流的客观规律性。结果表明:翼栅翼型头部流速和压力急剧变化,尾部出现流涡尾迹,前部是负压区,后部是正压区,内部流速大,压力小;在1/3弦长附近翼栅翼型表面压力出现拐点,拐点之前翼型上下表面压力差较大,拐点之后翼型上下表面压力差较小;翼栅内部流场具有相似、相近性,外部流场差异性较大;翼型的压力差是产生升力的主要原因。     

机动输油管线泄漏监测技术

机动输油管线采用露天方式快速铺设,容易发生泄漏事故。根据负压波原理,利用一种基于可变窗长中值滤波器的泄漏检测算法,在不降低检测灵敏度的前提下,能有效降低泄漏误报率。该算法在保证泄漏定位精度的同时,还能保持较高的实时性,较好地满足机动输油管线泄漏监测的需要。     

基于能量度量的星载AIS信号自适应码元同步抽取算法

基带信号码元同步抽取是目前星载AIS(Automatic Identification System)信号处理中的一个难点问题,针对过零检测和迟门早门等现有算法存在的不足,提出了基于能量度量的基带信号自适应码元同步抽取算法。将基带信号根据采样率和码速率的比值分割成相同的段的组合,之后分别计算每个段内相应样点的能量度量,最后选择使能量度量最大时的样点集作为最优同步抽取样点,该样点集具有最大信噪比。仿真结果验证了该算法误码率优于过零检测和迟门早门算法。     

基于信息论的C3I系统决策性能的评价

信息熵是描述信息系统的一种比较成功的方法.采用信息论的方法对决策系统进行描述,在考虑了决策者的有界合理性限制和达到满意性能指标的要求下,分析了单人指挥决策系统的系统性能,并在此基础上分析了多人指挥决策系统的系统性能,最后得出采用决策系统的误差概率P和相互一致性度量Q作为评价C3I系统决策性能标准的结论.     

Theoretical and numerical simulation study on jet formation and penetration of different liner structures driven by electromagnetic pressure

The use of a shaped liner driven by electromagnetic force is a new means of forming jets. To study the mechanism of jet formation driven by electromagnetic force, we considered the current skin effect and the characteristics of electromagnetic loading and established a coupling model of"Electric—Magnetic—Force"and the theoretical model of jet formation under electromagnetic force. The jet formation and penetration of conical and trumpet liners have been calculated. Then, a numerical simulation of liner collapse under electromagnetic force, jet generation, and the stretching motion were performed using an ANSYS multiphysics processor. The calculated jet velocity, jet shape, and depth of penetration were consistent with the experimental results, with a relative error of less than 10％. In addition, we calculated the jet formation of different curvature trumpet liners driven by the same loading condition and ob-tained the influence rule of the curvature of the liner on jet formation. Results show that the theoretical model and the ANSYS multiphysics numerical method can effectively calculate the jet formation of liners driven by electromagnetic force, and in a certain range, the greater the curvature of the liner is, the greater the jet velocity is.     

Investigate the effects of magnetic fields on the penetration ability of a shaped charge jet at different standoffs

The influence of a magnetic field on the stability of a shaped charge jet is experimentally investigated at standoffs of 490, 650 and 800 mm. The experimental results without and with the magnetic field are compared in terms of the shaped charge jet form, stability and penetration ability. A theoretical model based on one-dimension fluid dynamics is then developed to assess the depth of penetration of the shaped charge at those three standoffs and magnetic conditions. The results show that the penetration capability can be enhanced in more than 70% by the magnetic field. The theoretical calculations are compared with the experimental results with reasonably good correlation. In addition, the parameters introduced in the theory are discussed together with the experiments at three standoffs studied.     

Walker星座自主定轨误差分析

通过对Walker星座中卫星间的相对运动进行分析,给出星间相对距离的解析表达式及其对轨道根数的偏导数,直观地描述在同轨道面和异轨道面的星间观测对轨道根数变化的体现情况;根据星座中卫星的相对位置,提出合理的约束条件和平差方法,利用星间测距网实现星座的整网定位;通过仿真算例,比较在不同情况下,采用合适的整网定位方法对轨道根数的系统误差和随机误差修正的情况。