磁致伸缩扭转导波小管径弯管检测

针对扭转导波对小管径弯管的检测问题,分别采用数值模拟和实验方法进行研究。使用ANSYS软件模拟扭转导波在弯管中的传播;设计一种针对小管径管道的磁致伸缩扭转导波检测传感器,并对弯管进行检测,建立该传感器的导波激发和接收模型,利用理论模型对实验信号进行解读。研究结果表明:T(0,1)模态导波在小管径管道弯头处发生模态转换,部分T(0,1)模态转换成F(1,1)模态,F(1,1)模态具有方向性,垂直于弯头拱背-拱腹方向;模态转换会造成检测信号的双端面反射现象,第二个端面回波与第一个端面回波幅值比随频率的增大呈减小趋势;传感器激发出的纵向磁致伸缩力会导致实验信号中出现少量纵向模态导波。研究结论为磁致伸缩扭转导波对小管径弯管的检测提供理论指导。     

电磁轨道发射中内弹道动力响应特性分析

将轨道简化为移动载荷作用下固定在弹性支撑上的Bernoulli-Euler梁,通过静态电磁-结构耦合有限元模型求得外围封装的等效刚度,计算得到发射器的临界速度。另外,利用混合有限元/边界元法建立电磁-结构-运动多物理场耦合的动力学模型,求得枢轨动态接触压力和轨道的应力应变分布特性。通过在轨道背面布置光纤光栅应变传感器,利用测量数据验证了动力响应特性,并分析了弹丸在内弹道的稳定性。针对典型30 mm × 30 mm矩形口径发射器,分析及试验结果表明：C型电枢对轨道的电磁挤压力在平顶沿起始时刻达到最大值,之后随着时间推移逐渐减小;电枢通过引起的应力波在高速段容易与轨道中反射应力波发生共振,并且轨道在电枢运动的中间高速段区域受力最为集中,应力集中水平约是起始低速段区域的2.44倍;电枢运动高速段会出现晃动现象,进而引起上下轨道受力的不对称性。分析及试验结果对研究电磁轨道发射器内弹道动力响应特性和发射器结构设计具有重要指导意义。     

超声速燃烧火焰放热区结构CH-PLIF成像技术

超燃冲压发动机是吸气式高超声速飞行器的关键部件之一,超燃冲压发动机燃烧室内火焰结构的研究对揭示超声速燃烧的稳焰机理具有重要意义。利用平面激光诱导荧光（Planar Laser-Induced Fluorescence,PLIF）技术测量了超声速燃烧直连式试验台燃烧过程中重要自由基CH的二维分布,实现了超声速燃烧火焰放热区结构的可视化。在开敞空间的低速射流火焰炉中使用甲烷/空气预混火焰对CH-PLIF技术进行了初步验证和系统优化,再利用CH-PLIF技术在凹腔稳焰的超燃直连台上实现了超声速燃烧火焰放热区结构的二维可视化,并与OH-PLIF和CH自发辐射测量结果进行了对比。实验结果表明,在开敞空间的低速射流预混火焰中,火焰放热区会发生扭曲、褶皱和分裂等现象,随着雷诺数的增大,火焰锋面褶皱程度更加显著;在凹腔稳焰的超声速燃烧中,火焰放热区高度褶皱和破碎,放热区结构的厚度为0.5～6.5 mm,同时也存在放热区的分裂与剥离等现象。CH-PLIF技术能够以较高的空间分辨率更准确地呈现凹腔超声速火焰放热区的结构,其在凹腔稳焰的超声速燃烧诊断中具有重要的应用价值。     

超声速气流中液体横向射流一次破碎过程

发展显微成像方法获得空间分辨率为1.57 μm/pixel的近场射流瞬态图像,分析超声速气流中液体横向射流表面波演化规律。采用流体体积法获得射流的三维形态及近场流场特征,研究近场流场结构及气液作用。射流的一次破碎过程主要有表面破碎和液柱破碎。其中表面破碎由气液剪切引起的K-H不稳定主导,液柱破碎由气液加速引起的R-T不稳定主导;射流柱表面局部压力的脉动是诱导产生射流迎风面表面波并促使其沿射流方向发展的主要原因;射流柱与超声速气流作用形成背风面回流,近壁面液雾主要由表面破碎及背风面回流输运的液滴组成。     

Numerical simulation of the blast wave of a multilayer composite charge

The numerical simulation of a blast wave of a multilayer composite charge is investigated. A calculation model of the near-field explosion and far-field propagation of the shock wave of a composite charge is established using the AUTODYN finite element program. Results of the near-field and far-field calculations of the shock wave respectively converge at cell sizes of 0.25–0.5 cm and 1–3 cm. The Euler––flux-corrected transport solver is found to be suitable for the far-field calculation after mapping. A numerical simulation is conducted to study the formation, propagation, and interaction of the shock wave of the composite charge for different initiation modes. It is found that the initiation mode obviously affects the shock-wave waveform and pressure distribution of the composite charge. Additionally, it is found that the area of the overpressure distribution is greatest for internal and external simultaneous initiation, and the peak pressure of the shock wave exponentially decays, fitting the calculation formula of the peak overpressure attenuation under different initiation modes, which is obtained and verified by experiment. The difference between numerical and experimental results is less than 10%, and the peak overpressure of both internal and external initiation is 56.12% higher than that of central single-point initiation.     

Experimental research on the instability propagation characteristics of liquid kerosene rotating detonation wave

In order to study the instability propagation characteristics of the liquid kerosene rotating detonation wave (RDW), a series of experimental tests were carried out on the rotating detonation combustor (RDC) with air-heater. The fuel and oxidizer are room-temperature liquid kerosene and preheated oxygen-enriched air, respectively. The experimental tests keep the equivalence ratio of 0.81 and the oxygen mass fraction of 35% unchanged, and the total mass flow rate is maintained at about 1000 g/s, changing the total temperature of the oxygen-enriched air from 620 K to 860 K. Three different types of instability were observed in the experiments: temporal and spatial instability, mode transition and re-initiation. The interaction between RDW and supply plenum may be the main reason for the fluctuations of detonation wave velocity and pressure peaks with time. Moreover, the inconsistent mixing of fuel and oxidizer at different circumferential positions is related to RDW oscillate spatially. The phenomenon of single-double-single wave transition is analyzed. During the transition, the initial RDW weakens until disappears, and the compression wave strengthens until it becomes a new RDW and propagates steadily. The increased deflagration between the detonation products and the fresh gas layer caused by excessively high temperature is one of the reasons for the RDC quenching and re-initiation.     

Analysis of the stress wave and rarefaction wave produced by hypervelocity impact of sphere onto thin plate

Shock wave is emitted into the plate and sphere when a sphere hypervelocity impacts onto a thin plate. The fragmentation and phase change of the material caused by the propagation and unloading of shock wave could result in the formation of debris cloud eventually. Propagation models are deduced based on one-dimensional shock wave theory and the geometry of sphere, which uses elliptic equations (corresponding to ellipsoid equations in physical space) to describe the propagation of shock wave and the rarefaction wave. The “Effective thickness” is defined as the critical plate thickness that ensures the rarefaction wave overtake the shock wave at the back of the sphere. The “Effective thickness” is directly related to the form of the debris cloud. The relation of the “Effective thickness” and the “Optimum thickness” is also discussed. The impacts of Al spheres onto Al plates are simulated within SPH to verify the propagation models and associated theories. The results show that the wave fronts predicted by the propagation models are closer to the simulation result at higher impact velocity. The curvatures of the wave fronts decrease with the increase of impact velocities. The predicted “Effective thickness” is consistent with the simulation results. The analysis about the shock wave propagation and unloading in this paper can provide a new sight and inspiration for the quantitative study of hypervelocity impact and space debris protection.     

高频地波超视距雷达述评

高频(HF)地波超视距雷达(GW-OTHR)利用雷达波束绕地表面衍射作用,能探测视距外的舰船、低空飞机和巡航导弹,不仅覆盖面积大、费用低,能弥补常规微波雷达低空盲区和天波超视距雷达的近距盲区,也无需注意电离层的变化,且可反隐身、抗反辐射导弹(ARM),因而在许多国家的国民经济和国防领域中得到了广泛的应用。论述了地波沿海面传播的特性和探测能力,并对超视距雷达的发展和应用进行了介绍。     

高速方尾水面舰船兴波问题计算方法研究

将Dawson型兴波阻力计算方法推广用于高速方尾水面舰船兴波问题计算,在计算中同时计入了尾封板0静压力、尾倾与下沉等因素的影响.以两高速方尾水面舰船为例计算了兴波问题,将兴波阻力计算值与剩余阻力模型试验值进行了比较,求出了相应的相关系数.结果表明,本方法可较好地求解高速方尾水面舰船的兴波问题,兴波阻力相关系数可用于修正理论计算结果,以提高计算精度.     

雷电回击地面水平电场的解析求解

假定大地为良导电平面 ,基于DU模型计算了雷电回击地面电磁场 ,并探讨了地面水平电场的求解。对于雷电回击水平电场的两种近似求解方法———大地表面阻抗法和斜波法 ,进行了解析推导 ,并从数学上证明了两种方法在远区场的等价法。