低RCS飞行器外形设计实践

 在鸭式布局的基础上 ,对飞行器各部件及部件间的连接方式进行了外形隐身设计。对初步形成的鸭翼 -翼身融合体改变机身头部形状和立尾配置等进行 RCS优化。给出了飞行器各种状态下的 RCS平均值和迎头± 45°区内的 RCS值。测试结果表明 ,尖头机身、 30°双立尾 (立尾与垂直平面成± 30°角 )的鸭翼 -翼身融合体的 RCS值最小。对 RCS优化后的外形 ,风洞测力试验表明其气动性能也较好 (最大升阻比达到 8,失速迎角超过 2 6°)     

镍基高温合金铸件的晶粒组织控制──添加剂的影响

选用ＩＮ７３８ＬＣ镍基高温合金,研究了向熔体中加入碳化物、氮化物、硼及金属间化合物对合金冷凝后的晶粒尺寸、枝晶组织和初生碳化物形态等凝固组织特征的影响。结果发现,加入金属间化合物并控制合金液的均匀化处理过程可显著细化晶粒,并且对合金的结晶特性及凝固组织无不良影响。     

尖前缘翼干扰区的壁面压力和热流率分布

本文给出Ｍ＿∞＝７．８和６．７２，Ｒｅ＝３．５×１０￣７／ｍ和５．４×１０￣７／ｍ气流绕迎角为２０°、３０°和３５°尖前缘翼运动时，平板锥型干扰区的壁面压力和热流率分布。结果表明：（１）平板锥型干扰区的特征几何尺度与无粘激波角β＿０和翼迎角α相关，而壁面压力和热流率的峰值与法向马赫数Ｍ＿ｎ相关。（２）翼面压力和热流率分布由于受拐角涡影响，前者在翼根部呈波谷状，而后者呈波峰状，影响尺度与翼前缘处来流边界层厚度有关。     

Cosmic ray modulation in the 3-D heliosphere

The basic physical processes that lead to the long-term modulation of cosmic rays by the solar wind have been known for many years. However our knowledge of the structure of the heliosphere, which determines which processes are most important for the modulation, and of the variation of this structure with time and solar activity level is still incomplete. Study of the modulation provides a tool for probing the scale and structure of the heliosphere. While the Pioneer and Voyager spacecraft are surveying the radial structure and extent of the heliosphere at modest heliographic latitudes, theUlysses mission is the first to undertake a nearly complete scan of the latitudinal structure of the modulated cosmic ray intensity in the inner heliosphere (R<5.4 AU).Ulysses will reach latitudes of 80°S in September 1994 and 80°N in July 1995 during the approach to minimum activity in the 11 year solar cycle. We present a first report of measurements extending to latitudes of 52°S, which show surprisingly little latitudinal effect in the modulated intensities and suggest that at this time modulation in the inner heliosphere may be much more spherically symmetric than had generally been believed based upon models and previous observations.     

Ulysses out-of-ecliptic observations of “27-day” variations in high energy cosmic ray intensity

We report the discovery that for latitudes above 40°S, the observed recurring modulation of cosmic rays and anomalous nuclei occurs without the detection byUlysses of the solar wind velocity and magnetic field recurring enhancements that have, heretofore at lower latitudes, defined corotating interaction regions—i.e., the mechanism producing the recurring intensity variations >40°S appears to be located beyond the radial range ofUlysses.     

火箭发动机－超音速扩压器－蒸汽引射泵组合式高空模拟试验系统的性能研究

通过对火箭发动机－超音速扩压器－蒸汽引射泵组合式高模拟系统的理论分析和实验研究，提出了扩大ＧＳ－１高空模拟试车台试验能力的几项新方案。     

空腔倾向对泄漏影响的流动分析

给出了前倾斜腔，矩形空腔和后倾斜腔三种结构的四空腔迷密封实验结果。通过数值求解非定常Ｎ－Ｓ方程，预测上述三种结构的单空腔迷宫通道的内部流动，计算结果表明：后倾斜腔结构内部是稳态流动，而对于前斜腔和矩形空腔结构，流动表现为总体结构的基本稳定和局部结构的不稳定，局部不稳定的强弱顺序依次是前倾斜腔，矩形腔和后倾斜腔的迷宫结构。通过分析局部结构不稳定对减小泄漏的作用机制，说明不稳定效应的强弱是造成密封效果     

固体火箭燃烧室内微粒分布的实验研究

介绍一种实时脉冲取样器用于测定固体火箭燃烧室内凝相微粒尺寸分布技术，实验结果表明，含铝推进剂微粒呈二模态或三模分布，燃烧室内压力大，微粒趋大，燃烧室压力很小，微粒亦趋大，有一最小尺寸的压力值，残渣影响微粒尺寸测量，而推进剂燃烧特性将直接影响着微粒尺寸分布。     

超音速燃烧二元流场的数值模拟

由二元超音速燃烧流场垂直喷射Ｈ２的数值模拟计算，描述了缝隙喷嘴附近氧气与空气的混合和燃烧过程，使用两步化学反应，ＭａｃＣｏｒｍａｒｋ显式时间分裂法和Ｂａｌｄｗｉｎ－Ｌｏｍａｘ修正的代数湍流模型，计算超音速燃烧流场，得出了流线，静压，静温，Ｈ２和Ｈ２Ｏ浓度等值线图，反映了缝隙喷嘴附近回流区的大小，自动着火点的位置及火焰向主流的传播现象。     

固体发动机推力随机调节的涡流阀方案研究

介绍了一种固体发动机推力大小随机调节实现的方案－涡流阀方案，导出了涡流阀调节性能的相似准则方程；对涡流阀调节固体发动机静态特性和影响调节性能的各种主要因素进行了分析，指出了提出调节性能的途径，诸了模型发动机的推力调节。