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301.
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P.H. Krisko M. Horstman M.L. Fudge 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(7):1138-1146
In this paper we revisit the 1995 Kaman database of the SOCIT4 fragment characteristics with added analysis of a subset of the cataloged fragments from the test. This database was compiled from the last of a series of four hypervelocity impact tests conducted under a U.S. Department of Defense program in 1991–1992. This test targeted a flight-ready, U.S. Transit navigation satellite, yielding collision fragments in the size regime of sub-millimeter through tens of centimeters. Results in this database were used in the 1998 NASA Standard Breakup Model to represent characteristic length (size) and area-to-mass distributions of fragments smaller than 10 cm. 相似文献
303.
Long-duration spacecraft in low earth orbit such as the International Space Station (ISS) are highly susceptible to high-speed impacts by pieces of debris from past earth-orbiting missions. Among the hazards that accompany the penetration of a pressurized manned spacecraft are critical crack propagation in the module wall, crew hypoxia, and uncontrolled thrust due to air rushing out of the module wall hole. A Monte Carlo simulation tool was used to determine the effect of spacecraft wall construction on the survivability of ISS modules and crew following an orbital debris penetration. The simulation results indicate that enhanced shield wall designs (i.e., multi-wall systems with heavier inner bumpers) always lead to higher overall survivability of the station and crew due to an overwhelming decrease in likelihood of module penetration. The results of the simulations also indicate that changes in crew operations, equipment locations, and operation procedures can significantly reduce the likelihood of crew or station loss following an orbital debris penetration. 相似文献
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305.
飞机起落架载荷谱实测与编制方法 总被引:2,自引:0,他引:2
飞机起落架载荷谱实测时,应变计粘贴位置的选择是载荷谱实测的基础,然而起落架结构复杂,可供选择粘贴应变计的位置十分有限,因此研究并给出了起落架载荷谱实测时选择的典型测试切面,以为其他起落架载荷谱实测提供重要参考.根据实测载荷-时间历程,依据起落架受力特点对其进行了典型任务段的划分,分别对各个任务段进行载荷谱的编制.针对某... 相似文献
306.
多序列激光阴影成像技术研究及应用 总被引:3,自引:0,他引:3
为获取超高速碰撞过程中弹丸的飞行姿态及碰撞所产生的碎片云特性,开展了多序列激光阴影成像技术研究。利用多光源空间分离、偏振分光、光束角放大和补偿滤光等技术解决了单色光带来的衍射和干涉噪声以及碰撞瞬间强烈的自发光干扰问题,并先后在碰撞靶上建立了2序列、4序列和8序列激光阴影成像系统。该系统可以获得最小间隔1μs、曝光时间10ns、像素1000万的多个不同时刻的超高速瞬态变化过程图像,并在超高速碰撞靶试验中得到应用,获得了2~7km/s 撞击速度时碎片云的多序列阴影图像,该序列图像清晰地描述了碎片云的轮廓发展变化过程。该技术以低成本的方式实现了超高速摄影机的功能,满足目前碰撞试验粒子的飞行姿态及碎片云显示需要,并可以应用于其它超高速瞬态过程测量及流场结构显示。 相似文献
307.
针对航行体入水冲击过程中的流固耦合问题,利用任意拉格朗日 欧拉算法建立三维入水冲击数值仿真模型。首先,建立球体入水冲击数值模型,获取了入水过程中的冲击载荷和表面压力数据,通过与试验对比,探究网格密度、接触刚度耦合系数以及时间步长对仿真准确性的影响。结果发现,冲击区域网格密度和接触刚度耦合系数决定流固耦合接触刚度;冲击域的网状密度对冲击系数结果和入水速度变化有明显影响;耦合节点之间的接触刚度系数会影响局部压力峰值。最后,建立锥形头部圆柱体入水仿真模型,提出分段刚体计算截面载荷方法,研究不同速度下结构入水冲击加速度、速度、位移和截面载荷变化规律,与试验结果对比证明仿真准确性。 相似文献
308.
R. Hoogendoorn E. Mooij J. Geul 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):167-181
Predictions of the impact time and location of space debris in a decaying trajectory are highly influenced by uncertainties. The traditional Monte Carlo (MC) method can be used to perform accurate statistical impact predictions, but requires a large computational effort. A method is investigated that directly propagates a Probability Density Function (PDF) in time, which has the potential to obtain more accurate results with less computational effort. The decaying trajectory of Delta-K rocket stages was used to test the methods using a six degrees-of-freedom state model. The PDF of the state of the body was propagated in time to obtain impact-time distributions. This Direct PDF Propagation (DPP) method results in a multi-dimensional scattered dataset of the PDF of the state, which is highly challenging to process. No accurate results could be obtained, because of the structure of the DPP data and the high dimensionality. Therefore, the DPP method is less suitable for practical uncontrolled entry problems and the traditional MC method remains superior. Additionally, the MC method was used with two improved uncertainty models to obtain impact-time distributions, which were validated using observations of true impacts. For one of the two uncertainty models, statistically more valid impact-time distributions were obtained than in previous research. 相似文献
309.
S. Sen S. Carranza S. Pillay 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2010
The two primary requirements for a Martian habitat structure include effective radiation shielding against the Galactic Cosmic Ray (GCR) environment and sufficient structural and thermal integrity. To significantly reduce the cost associated with transportation of such materials and structures from earth, it is imperative that such building materials should be synthesized primarily from Martian in situ resources. This paper illustrates the feasibility of such an approach. Experimental results are discussed to demonstrate the synthesis of polyethylene (PE) from a simulated Martian atmosphere and the fabrication of a composite material using simulated Martian regolith with PE as the binding material. The radiation shielding effectiveness of the proposed composites is analyzed using results from radiation transport codes and exposure of the samples to high-energy beams that serve as a terrestrial proxy for the GCR environment. Mechanical and ballistic impact resistance properties of the proposed composite as a function of composition, processing parameters, and thermal variations are also discussed to evaluate the multifunctionality of such in situ synthesized composite materials. 相似文献
310.