基于复合疲劳试验的涡轮叶片振动应力反推法

提出了一种利用复合疲劳试验和外场故障数据反推涡轮叶片实际振动应力的方法.该方法针对与故障叶片同批次的叶片,开展数个振动应力水平下的单件试验和某一特定振动应力水平下的成组试验,利用极大似然法推导出叶片的概率-应力-寿命曲线(P-S-N);最后基于99.87%存活率下的概率-应力-寿命曲(P_99.87%-S-N),结合叶片的外场故障统计结果,反推出叶片实际工作中振动应力的范围和可能的最大振动应力.      

含能热塑性聚氨酯推进剂的能量计算与分析

采用最小自由能法,在标准条件(pc/p0=70∶1)下,比较了用不同软硬段结构的含能热塑性聚氨酯弹性体(ET-PU)作粘合剂的复合推进剂的能量特性,从要获得较高能量水平的观点,排列出了几种ETPU选择的先后次序;计算了含ETPU的各类推进剂的能量特性参数,探讨了ETPU对硝酸酯增塑的复合推进剂和硝胺改性双基推进剂的能量特性的影响规律。结果表明,选用不同ETPU的复合推进剂配方相互间在能量特性上存在着差别,但这种差别并不十分显著,以GAP为软段、TDI为硬段的ETPU,更有利于配方获得较高的能量水平;硝酸酯增塑的ETPU推进剂的理论能量水平高于丁羟推进剂,随增塑比逐渐增大,推进剂的最大理论比冲随之增大,固含量逐步降低;少量ETPU的加入,对硝胺改性双基推进剂的能量特性影响不大,增加Al和RDX含量,更有利于提高含ETPU的硝胺改性双基推进剂的能量水平。     

Designing method of acceleration and deceleration control schedule for variable cycle engine

Studies show that different geometries of a Variable Cycle Engine (VCE) can be adjusted during the transient stage of the engine operation to improve the engine performance. However, this improvement increases the complexity of the acceleration and deceleration control schedule. In order to resolve this problem, the Transient-state Reverse Method (TRM) is established in the present study based on the Steady-state Reverse Method (SRM) and the Virtual Power Extraction Method (VPEM). The state factors in the component-based engine performance models are replaced by variable geometry parameters to establish the TRM for a double bypass VCE. Obtained results are compared with the conventional component-based model from different aspects, including the accuracy and the convergence rate. The TRM is then employed to optimize the control schedule of a VCE. Obtained results show that the accuracy and the convergence rate of the proposed method are consistent with that of the conventional model. On the other hand, it is found that the new-model-optimized control schedules reduce the acceleration and deceleration time by 45% and 54%, respectively. Meanwhile, the surge margin of compressors, fuel–air ratio and the turbine inlet temperature maintained are within the acceptable criteria. It is concluded that the proposed TRM is a powerful method to design the acceleration and deceleration control schedule of the VCE.     

Integration of high-fidelity model of forward variable area bypass injector into zero-dimensional variable cycle engine model

Forward Variable Area Bypass Injector (FVABI) is one of key components which contributes to modulate the cycle parameters of Variable Cycle Engine (VCE) under various operation conditions. The modeling method of zero-dimensional FVABI was reviewed and its deficiency was analyzed based on FVABI flow characteristic. In order to improve the accuracy of VCE performance simulation, the high-fidelity modeling method of FVABI was developed based on its working characteristics. Then it was coupled with the zero-dimensional VCE model and the multi-level VCE model was built. The results indicate that the geometric and aerodynamic parameters can affect the interaction between the two airflows and the zero-dimensional FVABI model is too simple to predict the component performance accurately, especially when the FVABI inner bypass is chocked. Based on the performance curves for single bypass mode and the regression model of multi-scale support vector regression for double bypass mode, the high-fidelity model can predict FVABI performance accurately and rapidly. The integration of high-fidelity FVABI model into zero-dimensional VCE model can be done by adjusting iterative variables and balance equations. The multi-level model has good convergence and it can predict VCE performance when the FVABI inner bypass is chocked.     

火箭引射模态下主火箭总压与RBCC发动机的匹配性

基于传统的"等压面假设"理论,建立了RBCC发动机主火箭的引射性能分析模型,研究了主火箭总压与RBCC发动机的匹配性。研究结果表明,若隔离段通道面积比小于0.65,在主火箭总压较低条件下,隔离段内二次流容易达到壅塞,无法进一步提高空气流量;在地面静止状态下,随主火箭总压增加,空气流量逐步增大,等压面上形成Fabri壅塞后,进一步增加主火箭总压,反而会降低空气流量;在火箭引射模态下,RBCC发动机的工作状态可细分为引射作用占主导地位的进气道亚临界状态和临界状态、冲压作用占主导地位的进气道超临界状态,其分界马赫数分别约为0.7和1.5。     

行星轮系动态啮合应力研究

针对行星传动齿轮系的结构特点,建立了行星齿轮和主动齿轮的非线性接触有限元模型,应用AN-SYS软件进行了动态接触分析的研究。基于研究结果,建立了可以体现行星齿轮系在工作过程的啮合应力变化情况的计算模型,可以直观地观察到行星齿轮系从开始啮合到完全脱开整个过程中的应力分布及变化情况。选择20节点六面体单元,模拟齿轮受载情况,迅速、高效地得出整个齿轮系的强度、刚度分布云图,大大提高了设计效率。     

q-一致光滑Banach空间中的严格伪压缩映像

提出一种不用投影算子的修正的Mann遮代的循环算法,用于逼近q-一致光滑的Banach空间中有限个严格伪压缩映像的公共不动点,并证明了算法的强收敛性。本结论推广了Kim等和Zhang等关于非扩张映像的相应结果。     

内并联式TBCC进气道模态转换过程流动特性分析

针对组合动力(TBCC)进气道模态转换过程中出现的非定常气动现象,采用稳态/非稳态数值模拟方法对相关流动特性及其影响因素与流动机理开展了研究。结果表明：由涡轮发动机工作状态向冲压发动机工作模态转换过程中,进气道内出现结尾激波沿流向前后振荡现象,振荡频率约为130Hz;当冲压流道反压引起的激波未前传至模态转换分流板前时,冲压发动机工作状态对结尾激波振荡不产生影响。在相同的发动机工作状态下,随着模态转换速度的增加,结尾激波振荡频率逐渐增大。文中研究的进气道内结尾激波振荡现象可通过亚声速管道内波的传播理论进行解释和分析。     

空气预冷发动机及微小通道流动传热研究综述

首先针对发动机空气预冷系统的特点,将现有的预冷机制分为四种类型,包括燃料预冷、质量喷注预压缩冷却、燃料预冷和质量喷注预压缩冷却组合预冷以及其他流体预冷,并分别介绍了每种预冷机制的代表性发动机循环以及技术特点。调研发现,微小通道结构的预冷器具有很高的散热能力和紧凑度,优势显著。英国Skylon空天飞机的预冷却组合循环发动机（SABRE）其微通道结构预冷器具有极高换热能力。对SABRE的预冷器及相关研究进行详细分析,强调微小通道强化换热对提高发动机性能的重要作用。通过对微小通道中单相气态流动换热研究的调研发现,微尺度流动传热机理仍存在诸多分歧,理论发展不完善,需要深入开展微小通道强化传热研究,尤其对于高速高内外温差条件下微小尺度复杂结构空间内流动传热机理需要深入探索。     

Temporal and spatial variation of equatorial ionization anomaly by using multistation ionosonde data for the 19th solar cycle over the Indian region

The paper deals with the study of temporal and spatial variation of equatorial ionization anomaly (EIA) phenomenon along with its dependence on solar activity and season during the 19th solar cycle by using seven Indian ionosonde stations. Present study is an attempt to carry out the comprehensive study of EIA by using the limited number of ground based instruments. This has been achieved by performing the Gaussian fitting over the latitudinal distribution of F2-region critical frequency (foF2) data. Results reveal that the phenomenon of EIA has a strong dependence on solar activity and seasons. The EIA crest exhibits the feature of latitudinal shifting and expansion with increasing solar activity. It is found out that the effect of solar cycle and seasons on EIA is local time dependent. The observations were also compared with the IRI-2001 model predictions and results reveal that the model values are in general agreement with the observed values with some discrepancies, particularly during the high solar activity period and morning sector. The results have been discussed in the light of relative contribution from transequatorial interhemispheric neutral wind and strength of equatorial fountain process during different local time, season and solar activity levels. Furthermore, an attempt is made to parameterize the location and foF2 of the EIA crest by using the regression analysis. These results can be used to predict the latitudinal position and foF2 of the EIA crest for any given 12-month running average sunspot number (R12).