带多圈环形V型稳定器的加力燃烧室两态燃油浓度分布计算

在流场计算和油珠碰壁处理上进一步发展和完善了轨道扩散模型，编制了适用于具有多圈环形V型稳定器和多种喷油布置的加力燃烧室两态燃油浓度计算的通用程序。用于实际加力燃烧室的浓度场计算，可以给出加力燃烧室任意截面上液态、气态和总态燃油浓度分布，各区域内燃油浓度的平均值和周向平均燃油浓度沿径向的分布。     

复合材料层板多钉机械连接强度计算方法

提出了一种适于设计计算使用的复合材料层板多钉机械连接强度分析方法。该方法将复合材料板多钉机械连接强度分析问题化为求解各向异性体弹性理论中的复势函数边值问题,以Faber级数和最小二乘边界配置技术为工具导出了孔边应力的级数解表达式。选用的孔边特征曲线上的点应力失效判据避开了孔边接触、材料非线性、大位移、刚度减缩等复杂且难以验证的强度模拟计算过程。计算结果与试验结果符合较好。还详细探讨了铺层比例、排距等设计参数对钉载分配、挤压强度的影响规律。     

液体推进剂一甲肼与水二元物系汽液相平衡的研究

一甲肼是一种重要的液体推进剂,分离反应过程所生成的水是确保一甲肼质量的关键。测定了甲基肼－水（ＭＭＨ－Ｈ２Ｏ）物系在１０１．３３ｋＰａ下的汽液平衡,以及电解质对其汽液平衡的影响。采用盐效应和溶剂化的方法,研究了不同电解质对ＭＭＨ－Ｈ２Ｏ汽液平衡的盐效应。     

ADN 及其混合物燃烧性能的理论计算

分析了新型含能材料二硝酰胺胺（ＡＤＮ）的热分解特性和燃烧特性,提出ＡＤＮ燃烧初期热分解反应的假说,建立了由化学结构特征计算ＡＤＮ及其混合物燃速公式,并计算了ＡＤＮ和配比不同的ＡＤＮ混合物的燃速特征,计算结果与实测值十分一致。从化学结构和化学反应的层次分析了ＡＤＮ单质燃烧出现平台燃烧现象的原因,认为ＡＤＮ热分解过程中,中间产物ＮＨ４ＮＯ３的形成和消失在平台（麦撒）燃烧中起着关键作用,预测了ＡＤＮ提高     

固体火箭发动机绝热层缺陷对药柱燃面影响的数值模拟

发动机绝热层人工脱粘层局部产生缺陷时,经柱燃面曲线偏离设计曲线,导致发动机２内弹道性能也偏离设计为了模拟这种缺陷对药柱燃面的影响,扩展了原通用坐标程序地计算范围,并又新增加了一些基本图形的算法。改进后的算法可适用于绝热层有或没有缺陷的药柱燃面计算。针对绝热层缺陷建立了三种燃烧模型,计算分析了缺陷类型、结构与位置尺寸对药柱燃面的影响,为分析绝热层有缺陷的发动机性能的基础。     

双脉冲固体火箭发动机二次点火内视研究

利用Ｘ射线高速帝时荧屏分析（ＲＴＲ）技术对双脉冲固体火箭发动机的二次点过程进行了内研究,通过对ＲＴＲ图像的分析,弄清了隔板的打开模式以及塞子在一级燃烧室听运动规律,运用图像处理技术还获得了塞子飞出隔板后的平均速度及塞子与喷管碰撞后的反速度,这些结果为这种新型发动机的设计提供了实验依据。     

撞击平板的动力响应计算和实验研究

本文采用16节点立体等参元,进行了冲击速度为10～20m/s时的平板动力响应数值分析。程序中考虑了结构的大变形,采用全拉格朗日描述法,时间离散使用了纽马克法。文中分别对LY12CZ和PMMA两种材料平板的动力响应计算结果和试验结果作了比较。提出用HopkinsonBar装置测定平板在硬撞击下撞击总耦合载荷及撞击点挠度随撞击时间的分布关系。同时文中提供了上述两种材料的动态力学性能参数,由这些参数可以认为PMMA为应变率敏感材料,在高速撞击下呈现“脆化”现象,而LY12CZ则为应变率不相关材料,在冲击载荷下呈现良好的塑性变形特性。     

超高燃速固体推进剂研究概况

文中对多孔超高燃速推进剂(μ≥1000mm/s)的研究进展、多孔固体推进剂的研究内容、燃烧特性及有关配方作了介绍。最后总结了多孔超高燃速推进剂在密闭爆发器中和作为火炮随行装药的实验研究结果。     

Galileo Probe Nephelometer experiment

The objective of the Nephelometer Experient aboard the Probe of the Galileo mission is to explore the vertical structure and microphysical properties of the clouds and hazes in the atmosphere of Jupiter along the descent trajectory of the Probe (nominally from 0.1 to > 10 bars). The measurements, to be obtained at least every kilometer of the Probe descent, will provide the bases for inferences of mean particle sizes, particle number densities (and hence, opacities, mass densities, and columnar mass loading) and, for non-highly absorbing particles, for distinguishing between solid and liquid particles. These quantities, especially the location of the cloud bases, together with other quantities derived from this and other experiments aboard the Probe, will not only yield strong evidence for the composition of the particles, but, using thermochemical models, for species abundances as well. The measurements in the upper troposphere will provide ground truth data for correlation with remote sensing instruments aboard the Galileo Orbiter vehicle. The instrument is carefully designed and calibrated to measure the light scattering properties of the particulate clouds and hazes at scattering angles of 5.8°, 16°, 40°, 70°, and 178°. The measurement sensitivity and accuracy is such that useful estimates of mean particle radii in the range from about 0.2 to 20 can be inferred. The instrument will detect the presence of typical cloud particles with radii of about 1.0 , or larger, at concentrations of less than 1 cm³.Deceased.     

Energetic Particles Investigation (EPI)

The Energetic Particles Investigation (EPI) instrument operates during the pre-entry phase of the Galileo Probe. The major science objective is to study the energetic particle population in the innermost regions of the Jovian magnetosphere — within 4 radii of the cloud tops — and into the upper atmosphere. To achieve these objectives the EPI instrument will make omnidirectional measurements of four different particle species — electrons, protons, alpha-particles, and heavy ions (Z > 2). Intensity profiles with a spatial resolution of about 0.02 Jupiter radii will be recorded. Three different energy range channels are allocated to both electrons and protons to provide a rough estimate of the spectral index of the energy spectra. In addition to the omnidirectional measurements, sectored data will be obtained for certain energy range electrons, protons, and alpha-particles to determine directional anisotropies and particle pitch angle distributions. The detector assembly is a two-element telescope using totally depleted, circular silicon surfacebarrier detectors surrounded by a cylindrical tungsten shielding with a wall thickness of 4.86 g cm^-2. The telescope axis is oriented normal to the spherical surface of the Probe's rear heat shield which is needed for heat protection of the scientific payload during the Probe's entry into the Jovian atmosphere. The material thickness of the heat shield determines the lower energy threshold of the particle species investigated during the Probe's pre-entry phase. The EPI instrument is combined with the Lightning and Radio Emission Detector (LRD) such that the EPI sensor is connected to the LRD/EPI electronic box. In this way, both instruments together only have one interface of the Probe's power, command, and data unit.