机翼带外挂系统极限环颤振的区间分析

针对带有初偏间隙型非线性刚度的二元翼带外挂系统的极限环颤振,应用当量线化方法得出了颤振边界曲线,并根据颤振边界曲线用4阶Runge-Kutta法得到极限环相图,可明显看出极限环振动与普通周期振动的区别。然后引入了几个不确定量,通过区间分析方法给出了这些不确定量对机翼带外挂系统颤振边界曲线的影响,并用随机有限元法(FEM)验证区间分析方法的可靠性。进而可以得到一定来流速度下,具有不确定机翼外挂系统幅值的上下界,以及不确定参数对极限环相图的影响。知道机翼外挂幅值的上下界后,可以对外挂幅值进行适当控制。     

气-气冷流掺混流场缩尺技术

 为研究气-气冷流掺混流场缩尺技术,对多组分气相掺混流动三维Navier-Stokes无量纲方程及其定解条件进行了相似性分析,并将量纲分析方法应用到气-气掺混流动现象中,获得了气-气掺混流场相似准则,该相似准则表明冷流掺混试验件尺寸和试验背压都可以变化;运用该准则,在不同背压工况下进行了3个不同尺寸试验件的单喷嘴气-气喷注器掺混流场的仿真分析和比较,结果表明不同试验件尺寸和不同压力工况下气-气掺混流场具有相似性。研究结果能够指导气-气冷流试验,并为气-气燃烧流场缩尺技术研究提供参考。     

Prediction of fatigue crack growth rate for small-sized CIET specimens based on low cycle fatigue properties

Based on experiments of low cycle fatigue for 5083-H112 aluminum alloy, two energy-based predictive models have been introduced to predict the fatigue crack growth behaviors of traditional Compact Tension (CT) and small-sized C-shaped Inside Edge-notched Tension (CIET) specimens with different thicknesses and load ratios. Different values of the effective stress ratio U are employed in the theoretical fatigue crack growth models to correct the effect of crack closure. Results indicate that the two predictive models show different capacities of predicting the fatigue crack growth behaviors of CIET and CT specimens with different thicknesses and load ratios. The accuracy of predicted results of the two models is strongly affected by the method for determination of the effective stress ratio U. Finally, the energy-based Shi&Cai model with crack closure correction by means of Newman’s method is highly recommended in prediction of fatigue crack growth of CIET specimens via low cycle fatigue properties.     

高超声速串联式组合动力装置方案

为保证高超声速运输机在宽广的飞行包线内(Ma＝0~5,H=0~30km)稳 定可靠工作,对涡轮/冲压组合动力装置串联方案展开研究.首先建立了经试验数据校核的 适于高超声速飞行的组合动力装置部件级变循环详细非线性性能计算模型;在此基础上,利 用发动机设计点热力循环分析和非设计点性能分析方法对串联方案的综合特性进行评估,最 终给出一种经过优化的串联布局涡扇/冲压组合动力装置总体性能设计方案.研究结果表明 ,优化方案可有效地缩小组合发动机的结构尺寸与重量,有利于进气道,喷管的调节以及冲 压燃烧室燃烧的组织.通过综合调整发动机5个可调几何部位以及涡轮发动机燃油流量和冲 压燃烧室燃油流量,可以实现涡扇/冲压模式的平稳转换.      

气水分离器的修改设计与性能试验

本文是对航空发动机模拟试验台中的丝网分离器进行修改设计和试验工作的总结。着重叙述影响气水分离效率的重要参数——气流速度 V_D 的选择以及在结构上所做的改进,用试验方法验证设计达到了预期目的,并录取了分离效率与过网气速的关系曲线。     

PLC栈缓冲ASIC芯片的设计与实现

存贮管理是计算机体系结构的重要组成部分。对于Prolog和Lisp两种人工智能语言来说,它们的操作大多都是针对栈式存贮区进行的,因此一个高速的栈控制器将有效地提高它们的执行速度。本文简要介绍了Prolog/Lisp协处理器(PLC)栈缓冲机制的结构、原理以及栈缓冲专用芯片SC(Stack Controller)的设计方法和实现技术,为Prolog和Lisp语言的高效执行提供了一个性能价格比较高的存贮系统。     

保持时间对涡轮盘合金高温低周疲劳裂纹扩展特性的影响

研究了两种广泛使用的涡轮盘高温合金，在高温下带和不带上峰值保持时间的低周疲劳裂纹扩展特性及其扩展寿命估算模型。     

Solar and interplanetary precursors of geomagnetic storms in solar cycle 23

Estimating the magnetic storm effectiveness of solar and associated interplanetary phenomena is of practical importance for space weather modelling and prediction. This article presents results of a qualitative and quantitative analysis of the probable causes of geomagnetic storms during the 11-year period of solar cycle 23: 1996–2006. Potential solar causes of 229 magnetic storms (Dst ? −50 nT) were investigated with a particular focus on halo coronal mass ejections (CMEs). A 5-day time window prior to the storm onset was considered to track backward the Sun’s eruptions of halo CMEs using the SOHO/LASCO CMEs catalogue list. Solar and interplanetary (IP) properties associated with halo CMEs were investigated and correlated to the resulting geomagnetic storms (GMS). In addition, a comparative analysis between full and partial halo CME-driven storms is established. The results obtained show that about 83% of intense storms (Dst ? −100 nT) were associated with halo CMEs. For moderate storms (−100 nT < Dst ? −50 nT), only 54% had halo CME background, while the remaining 46% were assumed to be associated with corotating interaction regions (CIRs) or undetected frontside CMEs. It was observed in this study that intense storms were mostly associated with full halo CMEs, while partial halo CMEs were generally followed by moderate storms. This analysis indicates that up to 86% of intense storms were associated with interplanetary coronal mass ejections (ICMEs) at 1 AU, as compared to moderate storms with only 44% of ICME association. Many other quantitative results are presented in this paper, providing an estimate of solar and IP precursor properties of GMS within an average 11-year solar activity cycle. The results of this study constitute a key step towards improving space weather modelling and prediction.