超高速碰撞形成一次碎片云特性

对超高速碰撞数值模拟方法进行了讨论.采用ANSYS/AUTODYN程序的SPH方法,对球形弹丸超高速撞击时弹丸的破碎、碎片云的形成及扩展过程进行数值模拟,其结果与实验结果进行比较,并验证了计算方法和模型参数的正确性.在此基础上采用数值模拟方法,对钨合金、轧制均质装甲及LY12铝三种材料的球形弹丸超高速撞击靶板之后形成的一次碎片云形貌及演化规律进行了研究,并基于量纲分析方法得出了碎片云特征参数(碎片云头部速度、径向最大膨胀速度及膨胀角)随初始撞击条件的变化规律。     

双层反应装甲干扰射流影响因素分析

通过对双层反应装甲与射流作用过程进行分析和数值模拟,得到双层反应装甲飞板飞散及与射流作用物理过程,通过模拟结果与物理实验比较可知,数值模拟过程基本正确.同时,利用ANSYS-DYNA针对双层反应装甲不同结构参数与射流作用过程进行数值模拟,分析双层反应装甲两组件距离、与主靶板距离及两组件的夹角对干扰射流的影响,从而为双层反应装甲结构改进及设计优化提供理论参考.     

数值模拟金属靶抗侵彻中的网格密度影响研究

在数值模拟中,有限元网格的数量对计算结果和计算成本都有较大的影响。采用MSC.Patran建立了弹体侵彻金属靶板的计算模型,并利用MSC.Dytran对所建模型进行了计算;结合相关的理论,对不同网格密度划分的有限元模型的计算结果进行了分析,并和实验进行了对比,得到了数值模拟弹体侵彻金属装甲中靶板的最佳网格数量。当网格无因次量μ=0.10时,所得到的数值模拟结果与实际吻合得较好:当厚度方向的网格数取为12个时,文中所采用的模型能较好地模拟弹体对靶板的侵彻效果。     

平头弹丸侵彻金属靶板的数值仿真

基于ABAQUS/Explicit非线性有限元分析程序,通过二次开发利用含损伤的Johnson-Cook本构模拟靶板材料,对刚性平头弹丸垂直侵彻不同厚度的金属靶板进行了数值仿真,实现了侵彻过程的可视化。结果表明：网格密度对计算结果有影响,但随着网格密度增加,结果趋于收敛;侵彻过程中,弹丸与靶板发生了多次碰撞,靶板的塑性变形局限在很窄的剪切带内;对数值计算结果与试验结果进行了比较,发现二者吻合得较好。相关结论对防护结构的设计具有指导意义。     

填充式波纹夹层结构超高速撞击特性仿真

基于航天器空间碎片被动防护需求,对一种新型填充式波纹夹层结构进行超高速撞击仿真研究,分析超高速撞击过程以及结构的穿孔破坏情况和所形成的碎片云的特性,并与相同面密度Whipple结构进行对比。其撞击现象与Whipple结构相似,但其碎片云的头部速度小于Whipple结构,而径向膨胀最大速度和膨胀半角均大于Whipple结构。随撞击初速从3 km/s~10 km/s不断增大,波纹夹层结构的撞击穿孔尺寸变大,形状也更不规则。此外,结构中的填充树脂对碎片撞击能量的吸收贡献最大,后面板所吸收的能量所占比重较大,而前面板和波纹板对碎片撞击能量的吸收贡献较小。研究结果对空间碎片防护结构的设计具有一定的参考意义。     

爆炸成型弹丸侵彻靶板的数值仿真

基于LS-DYNA的动力学分析通用有限元程序,对爆炸成型弹丸形成和侵彻靶板过程进行了数值仿真。建立了数值仿真模型,利用数值模拟技术实现了弹丸的形成以及不同药型罩结构对爆炸成型弹丸形成的影响,实现了侵彻过程中弹丸的变形与靶板的破坏状况可视化,同时对仿真结果进行了分析。通过对爆炸成型弹丸侵彻靶板的数值仿真,为开展爆炸成型弹丸毁伤机理研究奠定了良好的基础。     

强爆轰驱动超高速碎片发射装置设计因素分析

为了得到发射装置设计因素和超高速碎片性能间的关系,考虑了药型罩的材料、炸药种类、装药长径比、药型罩的锥角、药型罩的厚度、药型罩顶部靠近装药侧的曲率半径等设计因素,采用AUTODYNTM,结合正交试验,对超高速碎片的发射过程进行数值模拟。结果表明,3种发射装置结构分别可以提供质量为1. 533 g的紫铜碎片、速度为11. 649 km/s的铝碎片、动能为85. 6 k J的铝碎片; 2种发射装置结构均可以提供质量大于1 g、速度高于11 km/s的密实结构圆柱状碎片。验证了仿真方法的可信性,对影响碎片性能的设计因素进行了分析、排序,并得到了这些设计因素与碎片质量、速度、动能的关系。     

爆炸冲击波对装甲车辆的毁伤效能

针对弹药爆炸对装甲车辆毁伤这一复杂问题进行了合理的简化,研究冲击波对靶板的作用过程。利用AUTODYN软件对爆炸冲击波对靶板的作用过程进行了数值模拟,分析了靶板前后空气压力的变化情况,得到爆炸冲击波作用下靶板中心的挠度值,并与理论计算结果相对比,二者具有良好的一致性,为下一步冲击波的毁伤效能研究提供参考。     

半穿甲战斗部侵彻运动加筋板数值模拟

为了研究加筋靶板的运动对半穿甲战斗部侵彻性能的影响,采用ANSYS/LS-DYNA有限元软件对截卵形半穿甲战斗部侵彻运动加筋靶板全过程进行了数值模拟,分析了在不同弹着点处加筋靶板的运动对弹体偏转、弹体剩余动能以及弹体过载的影响。研究结果表明:弹体侵彻运动加筋靶板时发生明显偏转,侵彻性能降低,加速度变化曲线出现新的峰值且该峰值随着靶板速度增大而增大。同时,不同弹着点处弹体偏转角的变化过程,加速度变化规律与峰值大小以及靶板抗弹性能都有显著区别。     

激光辐照下45#钢板响应特性

采取实验和数值模拟相结合的方法对激光辐照45#钢板的响应特性进行研究。基于连续光纤激光发射系统,开展钢板的激光辐照实验,得到温度场分布及靶板的烧蚀穿孔特性;基于ANSYS建立靶板有限元模型,模拟激光辐照下靶板的热响应过程,得到了靶板厚度、激光功率和光斑直径等因素对靶板温度分布及靶板穿孔特性的影响规律。     

Characteristics structure analysis on debris cloud in the hypervelocity impact of disk projectile on thin plate

In this paper, the gauge points setting is introduced in the SPH simulation to analyze the debris cloud structure generated by the hypervelocity impact of disk projectile on thin plate. Compared with the experiments, more detailed information of the debris cloud structure can be classified from the numerical simulation. However, due to the solitary dispersion and overlap display of the particles in the SPH simulation, accurate comparison between numerical and experimental results is difficult to be performed. To track the velocity and spatial distribution of the particles in the debris cloud induced from disk and plate, gauge points are locally set in the single-layer profile in the SPH model. By analyzing the gauge points’ spatial coordinate and velocity, the location and velocity of characteristic points in the debris cloud are determined. The boundary of debris cloud is achieved, as well as the fragments distribution outside the main structure of debris cloud.     

高速/超高速碰撞效应研究

高速/超高速碰撞会产生大量破片,并伴随闪光、等离子体等现象.高速碰撞材料受冲击产生射流及破片高温会引起碰撞闪光现象,获得了碰撞等离子体电磁场强度的变化规律.采用数值仿真与理论分析相结合的方法,获得了高速碰撞破片云团分布规律.     

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.     

Research and development on hypervelocity impact protection using Whipple shield: An overview

Whipple shield, a dual-wall system, as well as its improved structures, is widely applied to defend the hypervelocity impact of space debris (projectile). This paper reviews the studies about the mechanism and process of protection against hypervelocity impacts using Whipple shield. Ground-based experiment and numerical simulation for hypervelocity impact and protection are introduced briefly. Three steps of the Whipple shield protection are discussed in order, including the interaction between the projectile and bumper, the movement and diffusion of the debris cloud, and the interaction between the debris cloud and rear plate. Potential improvements of the protection performance focusing on these three steps are presented. Representative works in the last decade are mentioned specifically. Some prospects and suggestions for future studies are put forward.     

SPH数值模拟中固壁边界的一种处理方法

在光滑粒子流体动力学 (SPH)数值模拟中尝试了一种处理固壁边界的边界力方法 ,给出了一种新的边界力形式。利用SPH方法及边界力方法对水坝坍塌和涌波进入静止水塘这两个自由表面流动问题作了数值模拟。数值模拟结果表明 ,在SPH计算中使用本文所给边界力处理固壁是行之有效的     

Rayleigh-Taylor不稳定性的SPH模拟

采用SPH方法模拟了流体界面的Rayleigh Taylor不稳定性,给出了界面初始扰动的发展过程,得到了蘑菇状的扰动图像,并对两种不同初始分布的扰动过程进行了比较。分析表明,计算结果合理,SPH方法适合于界面不稳定性的模拟。     

基于FEM/SPH算法的弹丸侵彻土体数值模拟

基于有限元法(FEM)和光滑粒子流体动力学(SPH)结合的算法,用数值模拟了钢质弹丸对钢筒约束土体的侵彻过程。基于ANSYS/LS-DYNA显式动力分析和LS-PrePost后处理软件,形象再现了钢质弹丸冲击作用下土体飞溅形成漏斗坑和直线通道的物理过程。侵彻深度计算结果与实验数据吻合较好,钢质弹丸的速度和加速度时程曲线图与理论分析一致,体现了FEM/SPH算法的精确性。研究结果表明FEM/SPH算法在模拟侵彻土体方面具有可行性和有效性。     

Investigation on the spatial distribution characteristics of behind-armor debris formed by the perforation of EFP through steel target

The behind-armor debris (BAD) formed by the perforation of an EFP is the main damage factor for the secondary destruction to the behind-armor components. Aiming at investigating the BAD caused by EFP, flash X-ray radiography combined with an experimental witness plate test method was used, and the FEM-SPH adaptive conversion algorithm in LS-DYNA software was employed to model the perforation process. The simulation results of the debris cloud shape and number of debris were in good agreement with the flash X-ray radiographs and perforated holes on the witness plate, respectively. Three-dimensional numerical simulations of EFP's penetration under various impact conditions were conducted. The results show that, an ellipsoidal debris cloud, with the major-to-minor axis radio (a/b) smaller than that caused by shaped charge jets, was formed behind the target. With the increase of target thickness (h) and decrease of impact velocity (v₀) and obliquity (θ), the value of a/b decreases. The number of debris ejected from target is significantly higher than that from EFP. Based on the statistical analysis of the spatial distribution of the BAD, An engineering calculation model was established considering the influence of h, v₀ and θ. The model can with reasonable accuracy predict the quantity and velocity distribution characteristics of BAD formed by EFP.     

空间碎片碰撞风险评估模型及其应用

以现有的空间碎片环境模型为基础,建立了一套空间碎片风险评估模型。该模型包括空间碎片环境、航天器有限元建模、几何遮挡处理以及碰撞概率计算四个模块。为了验证风险评估模型的精度及有效性,针对机构间空间碎片协调委员会指定的三种标准工况,将该计算结果与国内外已有的风险评估模型的计算结果进行比较,验证了风险评估模型的正确性。利用开发的风险评估模型,对立方体航天器遭遇空间碎片碰撞风险进行仿真评估与分析,给出了轨道高度、倾角以及航天器自身的姿态参数对航天器遭遇空间碎片碰撞风险的影响特性。