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Performance of whipple shields at impact velocities above 9 km/s

机译:在9公里/秒以上的冲击速度下擦拭屏蔽的性能

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Whipple shields were first proposed as a means of protecting spacecraft from the impact of micrometeoroids in 1947 [1] and are currently in use as micrometeoroid and orbital debris shields on modern spacecraft. In the intervening years, the function of the thin bumper used to shatter or melt the threatening particles has been augmented and enhanced by the use of different types and configurations of intermediate layers of various materials. All shield designs serve to minimize the threat of a spall failure or perforation of the main wall of the spacecraft as a result of the impact of the particles. Various ballistic limit or "failure" equations for guiding the design and estimating the performance of Whipple shield systems have been developed. Most of these equations were developed in the 1960's and were used to estimate the performance of shields designed to provide protection against the extremely high impact velocities of micrometeoroids (11 km/s to 72 km/s). With the subsequent emergence of orbital debris as a more serious threat to spacecraft shielding, additional relationships were required for predicting the performance of shields impacted by lower velocity particles. Hayashida and Robinson [2] examined seven commonly used double-plate penetration equations for their accuracy and effectiveness in the development of shield designs. The best known and most used of the equations was the set of "new" modified Cour-Palais or Christiansen equations [3]. These equations were the only equations which addressed the three phases of impact: (1) ballistic (<3 km/s), where the projectile essentially penetrates as an intact projectile; (2) shatter (3 to 7 km/s), where the projectile fragments at impact and forms an expanding cloud of debris fragments; and (3) melt/vaporization (>7 km/s), where the projectile melts or vaporizes at impact. The results of 18 hypervelocity impact tests are presented in this paper. Thirteen test firings were made using three scales of a simple Whipple shield as targets and five test firings were made using a one-third-scale version of an all-aluminum Whipple shield installed on the U.S. Laboratory Module of Space Station as targets. The result of each test firing was compared to the appropriate ballistic limit curve generated for each of the shield designs. Six test firings, with impact velocities ranging from 6.94 to 7.28 km/s, were made using a two-stage, light-gas gun and twelve test firings, with impact velocities ranging from 8.75 to 9.89 km/s, were made using a three-stage, light-gas gun recently developed at the University of Dayton Research Institute (UDRI) [4].
机译:首先提出了奶屏蔽作为保护航天器免受Micrometeoroids在1947年的影响的手段[1],目前在现代航天器上用作微细象和轨道碎屑屏蔽。在介入年份中,用于粉碎或熔化威胁颗粒的薄保险杠的功能已经通过使用不同类型和各种材料的中间层的不同类型和构造来增强和增强。由于颗粒的影响,所有屏蔽设计都用于最大限度地减少航天器主壁的壁垒故障或穿孔的威胁。已经开发出用于指导设计和估算擦拭屏蔽系统性能的各种弹道限制或“故障”方程。这些方程中的大多数是在20世纪60年代开发的,用于估计屏蔽的性能,旨在为微晶体的极高冲击速度提供保护(11km / s至72公里/秒)。随着随后出现的轨道碎片作为对航天器屏蔽的更严重的威胁,需要额外的关系来预测由较低速度粒子影响的屏蔽的性能。 Hayashida和Robinson [2]检查了七种常用的双板穿透方程,以便在盾牌设计的开发中进行准确性和有效性。最着名的和最使用的等式是“新”修改的Cour-Palais或Christiansen方程的集合[3]。这些等式是解决了影响的三个阶段的唯一等式:(1)弹道(<3km / s),射弹基本上渗透到完整的射弹; (2)粉碎(3至7km / s),其中射弹碎片在撞击并形成碎片碎片的膨胀云; (3)熔化/蒸发(> 7km / s),射弹熔化或蒸发。本文提出了18个超高度影响试验的结果。使用三个简单的奶屏蔽的三个尺度制作了十三次测试烧制,以目标和五个测试燃烧是使用安装在U.S.的空间站实验室模块的全铝奶屏蔽作为目标。将每个测试烧制的结果与每个屏蔽设计产生的适当的弹道极限曲线进行比较。使用两阶段,轻气枪和12次试次射击的六个试速度,从6.94到7.28公里的冲击速度,使用三个速度从8.75到9.89 km / s的冲击速度。 - 最近在代顿研究所(UDRI)大学开发的轻气枪[4]。

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