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2019 15th Hypervelocity Impact Symposium最新文献

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Experiments using a light gas gun to investigate the impact melting of gunshot residue analogues 用轻气枪研究了枪弹残余物类似物的冲击熔化
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-030
V. Spathis, M. Price
In this set of experiments, the versatility of the University of Kent's light gas gun was utilised to obtain a selection of corroborative data regarding the formation and impact of metallic gunshot residues onto high purity silicon wafers. The results from the two experiments are presented. The first experiment investigated how the formation of metallic residues varied as gunshot residue analogues traversed through air under a range of pressures from 0.056 millibar (5.6 Pa) to 1 bar (100 kPa), using solely the energy released during primer ignition; the second involved firing a metallic powder mix of pre-determined composition (via a split-sabot) under vacuum at two velocities- 500 ms-1 and 2000 ms-1. This ensured that there was no ignition or heating of the powders, unlike the first experiment, and so the morphology of the particles collected would be solely due to impact. The residues on the substrates were then analysed using a cold Field Emission Gun Scanning Electron Microscope (FEG) and Energy Dispersive X-ray (EDX) detector. By separating the ignition process of the primers from the residue impacts, it allows for a closer look into the formation of these particles and helps determine whether their varied morphologies are due to the heating caused during the activation and combustion of the primer or whether its due to impact melting. This information can aid in the understanding of metallic particle formation in different pressure environments and give insight into the physical state of firearm residues when they impact a surface. Hydrocode modelling was also incorporated to corroborate the results observed during these experiments and gave results which mimicked the experimental data.
在这组实验中,肯特大学的光气枪的多功能性被用来获得关于金属射击残留物在高纯度硅晶片上的形成和影响的佐证数据。给出了两个实验的结果。第一个实验研究了在0.056毫巴(5.6 Pa)到1巴(100 kPa)的压力范围内,仅使用底火点火时释放的能量,射击残留物类似物在空气中穿行时金属残留物的形成是如何变化的;第二种方法是在真空条件下以两种速度——500ms -1和2000ms -1——发射预先确定成分的金属粉末混合物(通过分裂弹)。与第一次实验不同,这确保了粉末不会被点燃或加热,因此收集到的颗粒的形态将完全取决于撞击。然后使用冷场发射枪扫描电子显微镜(FEG)和能量色散x射线(EDX)探测器对衬底上的残留物进行分析。通过将底漆的点火过程与残留物撞击分离,可以更仔细地观察这些颗粒的形成,并有助于确定它们的不同形态是由于底漆激活和燃烧过程中引起的加热还是由于撞击熔化。这些信息有助于了解不同压力环境下金属颗粒的形成,并深入了解枪支残留物撞击表面时的物理状态。Hydrocode模型也被用于证实这些实验中观察到的结果,并给出了模拟实验数据的结果。
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引用次数: 0
Effects of EOS and constitutive models on simulating copper shaped charge jets in ALEGRA EOS和本构模型对ALEGRA中铜聚能射流模拟的影响
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-010
R. Doney, J. Niederhaus, T. Fuller, M. Coppinger
Metallic shaped charge jets (SCJ) have been studied for many decades across multiple communities for applications ranging from military warheads to earth penetrators for accessing oil-rich areas [1]. Researchers have had varied success in modeling these jets using simulation codes such as CTH, ALEGRA, and ALE3D. Recently, a large amount of work has been performed at the US Army Research Lab investigating the behavior of jets with increasingly sophisticated experimental diagnostics. Advances in computational resources, code enhancements, and material models have allowed us to model jets and probe uncertainties caused by algorithms, equations of state (EOS), constitutive models, and any of the available parameters each one provides. In this work we explore the effects that various EOS and constitutive models have on the development and characteristics of a 65-mm diameter, 2D copper SCJ using the Sandia National Laboratories’ multiphysics hydrocode, ALEGRA [2]. Specifically, we evaluate the tabular SESAME 3320 [3], 3325 [4-5], and 3337 [6] EOS models, analytic EOS (ANEOS) 3331 [7], as well as the Johnson-Cook (JC) [8], Zerilli-Armstrong (ZA) [9], Preston-Tonks-Wallace (PTW) [10], Steinberg-Guinan-Lund (SGL) [11-12], and Mechanical Threshold Stress (MTS) [13] constitutive models. Note that while the SGL model supports rate-dependence, there is no current characterization for copper, thus we are using rate-independent version. We do not consider the MieGrüneisen equation of state here as we expect parts of the jet to be near or cross into melt.
金属聚能射流(SCJ)已经在多个领域进行了数十年的研究,其应用范围从军用弹头到进入富油区的地球穿透器。研究人员使用CTH、ALEGRA和ALE3D等模拟代码对这些喷气机进行建模,取得了不同程度的成功。最近,美国陆军研究实验室进行了大量的工作,用越来越复杂的实验诊断来调查喷气机的行为。计算资源、代码增强和材料模型的进步使我们能够对射流进行建模,并探测由算法、状态方程(EOS)、本构模型和每个模型提供的任何可用参数引起的不确定性。在这项工作中,我们使用桑迪亚国家实验室的多物理场氢代码ALEGRA[2]探索了各种EOS和本构模型对65毫米直径2D铜SCJ的发展和特性的影响。具体而言,我们评估了表格式SESAME 3320[3]、3325[4-5]和3337 [6]EOS模型、解析式EOS (ANEOS) 3331[7],以及Johnson-Cook (JC)[8]、zerillii - armstrong (ZA)[9]、Preston-Tonks-Wallace (PTW)[10]、steinberg - guinian - lund (SGL)[11-12]和机械阈值应力(MTS)[13]本构模型。请注意,虽然SGL模型支持速率依赖,但目前还没有铜的特性描述,因此我们使用的是速率无关的版本。我们在这里不考虑米格-格- 尼森状态方程,因为我们预计射流的部分会接近或交叉进入熔体。
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引用次数: 0
Experiment guided simulation of multi-fragment impact into PBXs 实验指导下多碎片撞击pbx的模拟
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-108
A. Schmalzer, J. Yeager, P. Bowden, D. Guildenbecher, J. Olles
Multi-fragment impact of energetic materials can provide the impetus initiation and growth to detonation when shockwaves from these discrete fragments collide. The Sandia hydrocode CTH is used with reactive burn modeling to identify relationships between spherical fragment separation distances, variable fragment arrival timing, and initiability in energetic materials. This work demonstrates that detonation is most likely to occur is when multiple fragments collide with a surface simultaneously, because of the cumulative pressure rise of two equal colliding waves compared to the colliding waves generated by fragment impacts offset in time.
含能材料的多破片碰撞,当这些离散破片产生的冲击波相互碰撞时,可为爆轰提供起爆和增长的动力。Sandia hydrocode CTH与反应性燃烧建模一起用于识别含能材料中球形碎片分离距离、可变碎片到达时间和初始性之间的关系。本研究表明,当多个破片同时与一个表面发生碰撞时,最可能发生爆轰,这是由于两个相等的碰撞波的累积压力上升,而碎片撞击产生的碰撞波在时间上相抵消。
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引用次数: 0
Mesoscale modeling and debris generation in hypervelocity impacts 超高速撞击中尺度模拟与碎片生成
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-017
Stephanie N. Q. Bouchey, J. Hollenshead
Material fragmentation after a hypervelocity impact is of interest to predictive electro-optical and infrared (EO/IR) modeling. Successful comparisons with data require that submicron fragments are generated in such impacts; however, experimental data has so far been unable to produce fragments of this scale [e.g., 1-3]. This effort investigated the generation of predicted debris from hypervelocity impact of a sphere on a flat, semi-infinite plate. It is hypothesized that explicit modeling of grains, especially in the presence of void and varying grain properties, may lead to differences in predicted strain rates (locally higher) associated with the grain boundaries. Such an effect may lead to smaller predicted fragments sizes than when using the traditional bulk modeling approach and may provide improved understanding of fragmentation modeling in hypervelocity impacts. Comparisons of predicted strain rates at failure (a proxy for fragment size) and material temperature were made between simulations run using a bulk modeling approach and a mesoscale grain modeling approach.
超高速撞击后的材料碎裂是预测电光和红外(EO/IR)建模的重要内容。与数据的成功比较要求在这种撞击中产生亚微米碎片;然而,到目前为止,实验数据还无法产生这种规模的片段[例如,1-3]。这项工作研究了一个球体在一个平坦的半无限板块上的超高速撞击所预测的碎片的产生。假设晶粒的显式建模,特别是在存在空洞和不同晶粒性质的情况下,可能导致与晶界相关的预测应变率(局部较高)的差异。这种效应可能导致比使用传统块体建模方法时预测的碎片尺寸更小,并可能提高对超高速碰撞中碎片建模的理解。在使用体模型方法和中尺度颗粒模型方法进行的模拟中,比较了预测的失效应变率(碎片尺寸的代理)和材料温度。
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引用次数: 0
Transitional ballistics of electric high-velocity launchers 电动高速发射器的过渡弹道
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-092
B. Reck, S. Hundertmark, R. Hruschka, A. Zeiner, B. Sauerwein, M. Schneider
The high-velocity launch of a projectile is subjected to a number of disturbances which exert an influence on the flight trajectory. In the case of sub-caliber projectiles, sabot separation is one of the critical aspects. In this work, we focus on the projectiles and the launch package of an electric railgun launch, i.e. on the behavior of the launch-package, when transitioning from the gun barrel to free-flight. This work further addresses the use of a hydrocode for creating numerical models which are capable of predicting the motion and deflection of the sabot parts during their separation from the projectile after exiting the muzzle. An earlier study showed that the air flow around the projectile and the sabot can be modeled with sufficiently high accuracy by means of a simulation code that uses an Eulerian description of the gas flow. Within a time interval of several milliseconds, just the duration that a projectile needs to enter quasi-stationary flight, viscous effects of the air or gas flow have relatively little influence on the sabot discard process. If the Eulerian gas flow is coupled with the Lagrangian structural parts, the mechanical response of the latter to the gas pressure can be complex in terms of deformation and damage, and in that way, can affect the gas flow. In this study, the hydrocode model is applied to a medium caliber launch package concept for accelerating long rod projectiles. The computed results agree well with the corresponding experimental values obtained from a launch package model test in the shock tunnel at Mach 4.5. This demonstrates that the presented hydrocode model can be used for launch package design optimizations with high confidence.
弹丸的高速发射受到许多干扰,这些干扰对飞行轨迹产生影响。对于次口径弹丸,弹壳分离是关键问题之一。在这项工作中,我们重点研究了电轨道炮发射时的弹丸和发射包,即从炮管过渡到自由飞行时的发射包的行为。这项工作进一步解决了使用氢代码来创建数值模型的问题,该模型能够预测弹壳部分在离开枪口后与弹丸分离期间的运动和偏转。早期的研究表明,通过使用欧拉气体流动描述的仿真代码,可以以足够高的精度模拟弹丸和弹壳周围的空气流动。在几毫秒的时间间隔内,即弹丸进入准静止飞行所需的时间内,空气或气流的粘性效应对弹丸丢弃过程的影响相对较小。如果欧拉气体流动与拉格朗日结构部件耦合,则后者对气体压力的力学响应在变形和损伤方面可能是复杂的,从而影响气体流动。在本研究中,将氢码模型应用于中口径长杆加速弹丸的发射包概念。计算结果与4.5马赫激波隧道中发射包模型试验的相应实验值吻合较好。这表明所提出的氢码模型可用于发射包设计优化,具有较高的置信度。
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引用次数: 0
Impact Modeling for the Double Asteroid Redirection Test Mission 双小行星重定向试验任务的撞击建模
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-038
E. Rainey, A. Stickle, A. Cheng, A. Rivkin, N. Chabot, O. Barnouin, C. Ernst
The Asteroid Impact Deflection Assessment (AIDA) collaboration is a joint ESA-NASA planetary defense collaboration that will include the first full-scale test of an asteroid deflection by kinetic impactor [1]. The AIDA collaboration comprises two independent spacecraft, the NASA-sponsored Double Asteroid Redirection Test (DART) and the ESA-led Hera. In September 2022 the DART spacecraft will impact the secondary member of the binary asteroid system 65803 Didymos (Didymos-B) at a speed of ~6.7 km/s and mass ~500 kg. The resulting period change in the orbit of Didymos-B will be measured using Earth-based observations. Hera will arrive post-impact and perform detailed measurements to characterize Didymos-B.
小行星撞击偏转评估(AIDA)合作是esa和nasa联合开展的行星防御合作项目,其中将包括首次通过动力撞击器对小行星偏转进行全面测试[1]。AIDA合作包括两个独立的航天器,nasa赞助的双小行星重定向测试(DART)和esa领导的Hera。2022年9月,DART航天器将以6.7公里/秒的速度撞击双小行星系统65803 Didymos (Didymos- b)的次要成员。Didymos-B轨道的周期变化将通过基于地球的观测来测量。赫拉号将在撞击后到达,并对Didymos-B进行详细的测量。
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引用次数: 1
Automatic Mesh-Generation (FEM/SPH) for HVI-Simulations of Arbitrary Rotational Symmetric Impactors 任意旋转对称冲击器hvi仿真的自动网格生成(FEM/SPH)
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-080
Marvin Becker, M. Seidl, M. Mehl, M. Souli
For the numerical description of high velocity impact, Smooth-Particle-Hydrodynamics (SPH) has gained more and more interest. The standard Lagrangian Finite-Element (FE) approach has difficulties in describing large deformations and fracture. However, a simulation based on SPH only is very expensive due to the small size of the particles. A well adopted solution to this is to couple both methods, using SPH only where it is necessary, and capturing the outer boundary conditions with a bias FE-mesh correctly - without considerable extra computational cost. We apply such a hybrid approach in LS-DYNA® for the characterization of threats in terminal ballistics. Different meshing approaches for the projectile and target were implemented to guarantee an optimal initial condition. The particle size and the required size of the SPH-region were studied to exclude discretization effects. Exemplarily, a projectile surrogate with simplified geometry is investigated for a fixed impact velocity and two different angles of obliquity. A qualitative comparison between experiments, observed with X-ray cinematography, reveals a good potential of this approach towards predicting fracture and ricochet during high velocity impact events.
对于高速碰撞的数值描述,光滑粒子流体力学(SPH)得到了越来越多的关注。标准拉格朗日有限元(FE)方法在描述大变形和断裂时存在困难。然而,由于粒子尺寸小,仅基于SPH的模拟是非常昂贵的。一个很好的解决方案是将这两种方法结合起来,只在必要的地方使用SPH,并正确地用偏置fe网格捕获外部边界条件-没有相当大的额外计算成本。我们在LS-DYNA®中应用这种混合方法来表征终端弹道中的威胁。为保证初始条件的最优,对弹丸和目标采用了不同的网格划分方法。为了排除离散化效应,研究了sph区的粒径和所需粒径。举例来说,研究了一种几何简化的弹丸替代物,该替代物具有固定的冲击速度和两种不同的倾斜角度。通过x射线摄影观察到的实验间的定性比较,揭示了该方法在预测高速撞击事件中的断裂和弹跳方面的良好潜力。
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引用次数: 1
The Role of Inclusions in the Failure of Boron Carbide Subjected to Impact Loading 夹杂物在碳化硼冲击载荷失效中的作用
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-056
A. Tonge, B. Schuster
This work investigates the importance of the microstructure of boron carbide for initiating inelastic deformation under impact conditions. Simple loading resulting from a flyer plate impact geometry is used to illustrate the importance of microstructure for the well-controlled and easily instrumented experimental geometry. A second set of simulations is performed on a miniaturized impact geometry to investigate the importance of the microstructure for the early stages of semi-infinite penetration for impact velocities between 0.9 km/s and 1.9 km/s. The effect of the microstructure is more pronounced for the flyer plate impact geometry.
本文研究了碳化硼微观结构在冲击条件下引发非弹性变形的重要性。由飞片冲击几何形状产生的简单载荷被用来说明微观结构对于良好控制和易于仪器化的实验几何形状的重要性。第二组模拟是在一个小型化的冲击几何模型上进行的,以研究在0.9 km/s和1.9 km/s之间的冲击速度下,微观结构对半无限穿透早期阶段的重要性。微观结构对飞片冲击几何形状的影响更为明显。
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引用次数: 0
High velocity impact of an Fe/Cr/Mn/Ni high entropy alloy Fe/Cr/Mn/Ni高熵合金的高速冲击
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-008
M. Hawkins, S. A. Thomas, R. Hixson, Nan Li, S. Fensin
A series of shock loading experiments were conducted on High Entropy Alloy (HEA) samples consisting of Fe/Cr/Mn/Ni in weight percentages of 25.2/23.5/24.8/26.5. Characterizing this transition metal alloy is a first step in understanding the shock compression response of this relatively new class of alloy. A single stage light gas gun was used to conduct a series of flyer plate symmetric impact experiments to obtain fundamental dynamic properties. Photonic Doppler Velocimetry (PDV) diagnostics were employed to measure the free surface velocity on the back of each target during dynamic compression. These experiments yielded four data points that are in reasonable agreement with an estimated Hugoniot for the material.
对重量百分比为25.2/23.5/24.8/26.5的Fe/Cr/Mn/Ni高熵合金(HEA)试样进行了一系列冲击载荷试验。表征这种过渡金属合金是了解这种相对较新的合金的冲击压缩响应的第一步。采用单级轻气枪进行了一系列飞片对称冲击实验,获得了飞片的基本动力学特性。采用光子多普勒测速(PDV)诊断技术测量了动态压缩过程中每个目标背面的自由表面速度。这些实验产生了四个数据点,这些数据点与材料的估计Hugoniot基本一致。
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引用次数: 4
Hypervelocity impact performance of 3D printed aluminum panels 3D打印铝板的超高速冲击性能
Pub Date : 2019-04-14 DOI: 10.1115/hvis2019-055
B. Davis, Richard A. Hagen, Robert J. McCandless, E. Christiansen, D. M. Lear
NASA, JSC has been developing a light-weight, multi-functional sandwich core for habitable structure over the last several years. Typically honeycomb-based structures have been and still are a common structural component for many applications in the aerospace industry, unfortunately, honeycomb structures with an ordered, open path through the thickness have served to channel the micro-meteoroid or orbital debris into the pressure wall (instead of disassociating and decelerating). The development of a metallic open cell foam core has been explored to enhance the micro-meteoroid or orbital debris protection, which is heavier than comparable honeycomb-based structures when non-structural requirements for deep space environments (vacuum, micro-meteoroids/orbital debris, and radiation) have not been considered. While the metallic foam core represents a notable improvement in this area, there is an overwhelming need to further reduce the weight of space vehicles; especially when deep space (beyond low earth orbit, or LEO) is considered. NASA, JSC is currently developing a multi-functional sandwich panel using additive machining (3D printing), this effort evaluated the material response of a limited amount of 3D printed aluminum panels under hypervelocity impact conditions. The four 3D printed aluminum panels provided for this effort consisted of three body centric cubic lattice structure core and one kelvin cell structure core. Each panel was impacted once with nominally the same impact conditions (0.34cm diameter aluminum sphere impacting at 6.8 km/s at 0 degrees to surface normal). All tests were impacted successfully, with the aforementioned impact conditions. Each of the test panels maintained their structural integrity from the hypervelocity impact event with no damage present on the back side of the panel for any of the tests. These tests and future tests will be used to enhance development of 3D printed structural panels.
在过去的几年里,NASA、JSC一直在为可居住的结构开发一种轻质、多功能的夹层核心。典型的蜂窝结构已经并且仍然是航空航天工业中许多应用的常见结构部件,不幸的是,蜂窝结构在厚度上具有有序的开放路径,用于将微流星体或轨道碎片引导到压力壁上(而不是分离和减速)。在不考虑深空环境(真空、微流星体/轨道碎片和辐射)的非结构要求时,探索了金属开孔泡沫芯的开发,以增强对微流星体或轨道碎片的保护,比类似的蜂窝式结构更重。虽然金属泡沫芯是这方面的显著改进,但迫切需要进一步减轻空间飞行器的重量;特别是考虑到深空(低地球轨道或LEO之外)时。NASA, JSC目前正在使用增材加工(3D打印)开发多功能夹心板,这项工作评估了有限数量的3D打印铝板在超高速冲击条件下的材料响应。为这项工作提供的四个3D打印铝板由三个体心立方晶格结构核心和一个开尔文细胞结构核心组成。每个面板在名义上相同的冲击条件下撞击一次(0.34cm直径的铝球在与表面法线0度的情况下以6.8 km/s的速度撞击)。在上述冲击条件下,所有测试都成功进行了冲击。在超高速撞击事件中,每个测试面板都保持了其结构完整性,在任何测试中,面板的背面都没有出现损坏。这些测试和未来的测试将用于加强3D打印结构板的开发。
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引用次数: 0
期刊
2019 15th Hypervelocity Impact Symposium
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