共查询到17条相似文献,搜索用时 296 毫秒
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文章利用一组二级轻气炮发射2017-T4 铝质球形弹丸撞击6061-T6单层铝板的地面试验数据,通过选择适当的函数模型,采用多元函数拟合的方法,得到了碎片云前端速度与靶板厚度、弹丸直径和弹丸速度关系的三元二阶多项式模型。再用另外一组数据对该模型进行检验,验证了其对碎片云前端速度具有较好的预测效果。将以上两组数据同样用于建立“无量纲化”模型进行碎片云前端速度预测,并与前述多项式模型的预测结果进行比较发现,该多项式模型预测的方均根误差及平均相对误差均明显优于“无量纲化”模型。该多项式模型可用于预测空间碎片撞击航天器产生的碎片云的前端速度,有助于航天器的空间碎片防护设计。 相似文献
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超高速撞击弹丸形状效应数值模拟研究 总被引:3,自引:0,他引:3
为保证在轨航天器的安全运行,微流星体和空间碎片的防护成为现有航天器,特别是长寿命、大尺寸航天器设计时必须考虑的问题。本文采用AUTODYN软件进行了不同形状弹丸超高速撞击whipple防护结构的数值模拟,对不同形状弹丸撞击Whipple防护结构的撞击极限曲线进行了比较,分析了各形状弹丸撞击防护屏后形成的碎片云状态,以及分析了各撞击极限曲线之间差异的原因。不同形状弹丸对Whiple防护结构的损伤能力有很大差异,弹丸破碎和碎片云分散程度随弹丸速度、长径比和撞击方向的改变而改变。 相似文献
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超高速撞击中的弹丸形状效应数值模拟研究 总被引:2,自引:0,他引:2
文章用AUTODYN仿真软件对球形、圆锥形、圆柱形和盘形4种不同形状弹丸超高速撞击Whipple防护结构所产生的碎片云形貌特征及对后墙的毁伤程度进行了数值仿真研究。对比分析结果指出:质量与速度相等的4种不同形状弹丸撞击缓冲屏所产生的碎片云有明显差异;弹丸长径比越小,穿过缓冲屏后的破碎程度越大;在5 km/s撞击速度下,球形弹丸对后墙的毁伤程度最小,而圆柱形弹丸的毁伤程度最大。这说明弹丸的形状对超高速撞击结果有显著影响,在航天器超高速撞击风险评估和防护工程设计中应充分考虑弹丸的形状效应。球形弹丸的弹道极限曲线在防护结构的碎片防护能力评价时存在高估的问题,在实际工作中要特别注意这一点。 相似文献
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建立了一种航天器防护结构超高速碰撞数值模拟的节点分离有限元方法。通过重合节点网格转换和添加节点集约束建立了节点分离有限元模型。在显式积分迭代中,将达到断裂判据的节点集解离,从而生成裂纹。对网格畸变问题进行分析,并建立了几何识别方法,进而删除畸变单元,改善了算法的稳定性。应用节点分离方法模拟了单层板超高速撞击问题,并分析了撞击速度对弹丸变形程度和碎片云形状的影响。应用节点分离方法对Whipple防护结构、填充式防护结构和多层网结构进行了模拟,获得了与实验一致的结果。多种算例表明,节点分离有限元方法改善了以往断裂侵蚀有限元方法处理网格畸变、碎片云模拟以及二次碎片云碰撞等方面的能力,对典型防护结构模拟具有很好的适用性,能够成为光滑粒子流体动力学(SPH)方法的有效补充和替代。 相似文献
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球形弹丸超高速正撞击Whipple防护结构损伤分析 总被引:1,自引:0,他引:1
为了掌握航天器防护结构受空间碎片高速撞击的防护性能及其损伤破坏模式,采用二级轻气炮结合高速X光照相系统,对球形弹丸超高速正撞击5A06铝合金whipple防护结构进行了试验研究.根据试验结果分析了铝合金whipple防护结构的防护屏和舱壁在弹丸撞击速度为2.0-5.2km/s、弹丸直径为4mm和6.35mm及防护屏厚度为0.5film、1.5mm、2mm和3mm区间的损伤模式,总结了防护屏穿孔和舱壁损伤随弹丸撞击速度、弹丸直径以及防护屏厚度变化的规律.根据高速x光照片分析了碎片云速度和形态的变化趋势,进而从碎片云角度对舱壁损伤模式进行了分析. 相似文献
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提出了双层板防护结构的超高速碰撞数值模拟的工程算法模型,采取理论分析、经验公式和数值模拟相结合的研究方法来模拟碎片云的产生,以及碎片云对结构的破毁过程。本模型中,碎片云的产生采用理论分析和经验公式得到,结构响应采用有限元动力学软件Dyna3D进行计算。数值模拟结果与文献中给出的破坏效果基本一致,说明提出的工程算法是可行的,模拟得到的结果能定性的描述相应的超高速碰撞的现象,得到基本正确的结果。 相似文献
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Whipple shield is widely used on manned spacecraft, numerical simulation is an important way for obtaining the ballistic limit. The large population of particles and the large space span of Whipple shield simulation model restrict the computational efficiency. A fast numerical approach is presented for Whipple shield ballistic limit analysis. First, the critical penetration analysis of the rear walls is converted into specific impulse analysis delivered by the secondary debris cloud, because the maximum of specific impulse is the main determinant of the penetration. The dual plate simulation model is then converted into single plate model and the population of particles is reduced. Second, based on the isotropic expansion theory of secondary debris cloud, the specific impulse analysis is further converted into particle position and velocity analysis when the stable secondary debris formed. The space span of the simulation model is reduced. An example of Whipple shield ballistic limit analysis is provided for the verification of the fast numerical approach, it shows that this approach can significantly increase the computation efficiency with acceptable accuracy. 相似文献
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Sheng-wei Lan Sen LiuAuthor VitaeYi LiAuthor Vitae Fa-wei KeAuthor VitaeJie HuangAuthor Vitae 《Acta Astronautica》2014
Cross-sectional area is an important parameter for spacecraft breakup debris as it is the directly measured data in space observation. It is significant for observing and analysing the spacecraft breakup event to accurately modelling the area distribution of the breakup debris. In this paper, experimental study has been performed on debris area distribution characteristics of spacecraft under hypervelocity impact. The tests are carried out at the ballistic ranges of CARDC. Aluminium projectiles are launched to normally impact the simulated spacecrafts at about 3.0 km/s. The simulated spacecrafts are made up of aluminium plates, filled with some simulated electronics boxes, each of which was installed with a circuit board. “Soft-catch” devices are used to recover the breakup fragments. The test results show that: 1) the relationship between the cross-sectional area and the characteristic length of debris, which can be obtained in the logarithmic coordinates by linear fitting, represents the debris shape characteristic in a certain extent; 2) the area-to-mass ratios of fragments show normal distributions in the logarithmic coordinates; 3) debris made of different materials can be distinguished by different peaks on the distribution curves; 4) the area-to-mass ratio distributions can be expressed by a linear superimposition of several normal functions which represent the main materials of the spacecraft. 相似文献
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《Acta Astronautica》2009,64(11-12):1312-1317
This paper attempts to search the lost fragments from the near-synchronous US TitanIIIC transtage explosion of February 21, 1992, known as the second major fragmentation of a TitanIIIC transtage. This breakup was accidentally observed by the Maui GEODSS sensor, and then a total of 23 objects were reported from the breakup, no orbital data on any fragments has been generated by the SSN. In order to evaluate the debris cloud orbital evolution, we demonstrate the actual US TitanIIIC transtage explosion by using breakup model and orbit propagator. The perturbing accelerations, considered in this analysis are the non-spherical part of the Earth's gravitational attraction, the gravitational attraction due to the Sun and Moon, and the solar radiation pressure effects. Finally, we will present a search strategy based on distribution of the right ascension of the ascending node about the catalogued objects and the debris particles from the US TitanIIIC transtage explosion. 相似文献