液体火箭发动机推力室复合冷却流动与传热研究

为了预测液体火箭发动机推力室的复合冷却性能,建立了推力室再生冷却通道和超临界氢的三维仿真模型以及推力室内燃气和超临界氢膜的轴对称二维仿真模型。通过边界耦合发展了液体火箭发动机推力室复合冷却流动与传热的数值仿真方法。对航天飞机主发动机推力室内部燃气、超临界冷却膜、室壁和再生冷却剂进行了流动与传热耦合计算仿真研究。研究表明,仿真方法可较好地预测推力室燃气及再生冷却剂的流动和传热,计算得到航天飞机主发动机的燃气侧壁面最高热流密度为129MW/m2,最高壁温为885K,冷却剂温升为192K,压降为8.8MPa,结果与已有数据吻合较好。模型和仿真方法可用于液体火箭发动机推力室冷却系统传热计算和冷却结构的优化设计。     

液体火箭发动机推力室再生冷却流动与传热计算研究

为了研究液体火箭发动机推力室再生冷却流动与传热的快速仿真方法,建立了推力室再生冷却的准二维模型,对航天飞机主发动机开展了再生冷却流动与传热计算仿真研究,对比分析了再生冷却准二维模型和三维模型的仿真计算结果。研究表明,两种计算模型均可较好地预测推力室燃气及再生冷却剂的流动和传热。三维模型计算精度高,但计算用时较长。计算得到的航天飞机主发动机的燃气侧壁面最高热流密度为162.2MW/m2,最高壁温为1159.7K,冷却剂温升为244.0K,压降为8.5MPa。准二维模型计算结果精度略有降低,但计算时间较三维模型减小了90%。四个参数与三维模型计算结果的差异分别为0.3%,4.4%,8.6%和4.5%,在可接受范围内。本文的准二维模型计算时间短,适用于液体火箭发动机再生冷却结构的方案筛选和优化设计,三维模型计算精度高,适用于设计完成后的校核计算。     

液体推进剂火箭发动机推力室再生冷却通道三维流动与传热数值计算

应用湍流模型对液体推进剂火箭发动机再生冷却推力室通道的流动与传热进行了三维数值模拟,冷却工质为氢气,其密度、导热系数、动力粘度随着温度和压力而变化,冷却剂比热容及金属固体物性随着温度而变化。计算采用标准k-ε双方程湍流模型及气-固耦合算法。结果表明:推力室燃气侧壁面的温度和热流密度的最高点均发生在喉部附近,喉部横截面固体区域最大温度梯度靠近燃气,喉部附近氢气在垂直主流方向的截面上产生了二次流。气固耦合面最大热流密度及最大对流换热系数同样位于推力室喉部附近。      

气壁镀镍和冷却剂入口对再生冷却的影响

考虑冷却剂入口模型及气壁镀镍,对液体火箭发动机推力室再生冷却通道和冷却剂进行三维流动与传热耦合计算.采用经验公式计算燃气侧对流及辐射换热,冷却剂为甲烷,考虑其物性随温度和压力的变化.所得结果表明:冷却剂入口二次流及突扩流场的叠加,使局部压力损失变大,影响进口下游较大区域流动传热状况;气壁镀镍能提高气壁的耐高温性,降低气壁锆铜的温度.      

膨胀循环推力室再生冷却换热的数值模拟

为了解液体火箭发动机膨胀循环推力室再生冷却换热特性,采用数值模拟方法,研究了冷却剂流动方式、推力室圆柱段长度、圆柱段室壁加肋和气壁面粗糙度等因素对冷却通道压降、冷却剂温升、壁面热流密度和温度分布等换热特性的影响.计算过程中采用k-ε双方程湍流模型.计算结果表明:采取顺流冷却要比逆流冷却的冷却通道压降低,但同时冷却剂温升也低;对于室壁加肋结构,在肋个数相同而只改变肋高度的情况下,总换热量正比于总换热面积.      

液氧甲烷发动机台阶型冷却通道的耦合传热特性

为了研究液氧甲烷发动机再生冷却通道中跨临界甲烷的流动和传热特性,以及冷却通道较大幅度的突扩突缩对冷却效果的影响,采用整场直接耦合的方法对推力室三维耦合传热进行了数值模拟,考虑了燃气的非平衡流动.通过计算得到了推力室三维温度场和流场.计算结果表明：由于喉部截面附近存在较强的二次流,燃气侧壁面温度的最大值出现在喉部上游.由于突扩突缩处存在较强的旋涡运动,冷却剂的湍流强度增强,冷却剂侧表面传热系数显著提高,燃气侧壁面温度出现局部极小值,同时也产生了较大的局部损失.由于铜内衬热阻比镍外套热阻小得多,从燃烧室进入的大部分热量在冷却通道底面和侧面被冷却剂吸收.冷却通道底面的温度和热流密度沿程变化比顶面更剧烈.     

气气喷注器推力室传热特性研究

设计了单喷嘴气气喷注器容热式推力室,进行了0.92～6.1 MPa范围内7个燃烧室压力工况,共17次热试车;采用壁面测温方法获得推力室沿轴向方向的内壁热流分布,得到各室压工况下燃烧室内壁热流分布曲线,不同工况的热流曲线显示出相似的分布;并从中分离出对流传热热流,得到对流传热热流与室压的关系。为拓展范围,采用多组分湍流N-S方程描述推力室内燃烧流动,采用6组分9步反应模型来描述氢氧反应,反应速率由Arrhenius公式计算,进行了5～20 MPa更高室压范围内的燃烧内流场的数值模拟,并耦合计算了各工况燃气与室壁之间的传热,获得了与试验相同规律的结果。     

通道深宽比对液体火箭发动机推力室再生冷却的影响

应用湍流模型对液体推进剂火箭发动机再生冷却推力室通道的流动与传热进行了三维数值模拟, 冷却工质为氢气, 其密度、导热系数、动力粘度随着温度和压力而变化, 冷却剂比热容及金属固体物性随着温度而变化.计算采用标准k-ε两方程湍流模型及气-固耦合算法.保持再生冷却通道个数及冷却工质进口流量不变, 通过改变通道肋壁厚度来改变冷却通道深宽比, 研究不同深宽比对推力室壁面再生冷却效果的影响规律.计算结果表明:增加通道深宽比对推力室壁面能够起到强化传热的作用, 但同时也增加了冷却通道的进出口压差.这是由于冷却工质流速的增高, 从而提高了推力室传热系数.随着深宽比不断增加, 推力室再生冷却效果趋于饱和, 而冷却工质进出口压降则不断上升.      

燃气非平衡流再生冷却流动传热数值模拟

为准确预测液体火箭发动机推力室身部再生冷却换热状况,采用数值模拟方法,对燃气、推力室壁和超临界气氢进行三维流动和换热耦合计算。采用6组分9步反应动力学模型计算燃气的非平衡化学反应,采用DO模型计算燃气辐射换热,考虑超临界气氢物性随温度和压力的变化。获得了室壁温度场、燃气及冷却剂流场。结果表明,Redlich-Kwong方程、Peng-Robinson方程、Lucas法、TRAPP法能分别准确计算超临界氢的密度、定压比热容、粘度、导热系数,采用燃气非平衡流计算所得流场值更符合实际情况。     

冷却剂不同流动方式对膨胀循环推力室再生冷却换热的影响

为了解液体火箭发动机膨胀循环推力室再生冷却换热特性,对某一参考发动机推力室和另外两种面积比的膨胀循环推力室建立三维计算模型,采用数值模拟的方法,考察冷却剂的温升、冷却通道压降以及推力室内壁面温度和热流密度的分布情况.重点比较了不同燃烧室圆柱段长度、冷却剂不同流动方式以及不同面积比对以上结果的影响.计算过程中采用二阶迎风格式离散控制方程.计算结果表明:采用逆流冷却时,通过加长推力室圆柱段长度使推力室受热面积增加70%后,冷却剂温升提高了一倍左右;对膨胀循环推力室进行再生冷却时,采用顺流冷却要比逆流冷却的冷却通道压降低,但同时冷却剂温升也较低,并且对喉部壁面的冷却效果较差.     

The effect of inlet conditions on the flow and heat transfer in multiple rotating cavity with axial throughflow

This paper discusses experimental results from two different build configurations of a heated multiple rotating cavity test rig.Measurements of heat transfer from the discs and tangential velocities are presented.The test rig is a 70% full scale version of a high pressure compressor stack of an axial gas turbine engine.Of particular interest are the internal cylindrical cavities formed by adjacent discs and the interaction of these with a central axial throughflow of cooling air.Tests were carried out for a range of non-dimensional parameters representative of high pressure compressor internal air system flows(Re up to 5×106 and Rez up to 2×105).Two different builds have been tested.The most significant difference between these two build configurations is the size of the annular gap between the(non-rotating) drive shaft and the bores of the discs.The heat transfer data were obtained from thermocouple measurements of surface temperature and a conduction solution method.The velocity measurements were made using a two component,LDA system.The heat transfer results from the discs show differences between the two builds.This is attributed to the wider annular gap allowing more of the throughflow to penetrate into the cavity.There are also significant differences between the radial distributions of tangential velocity in the two builds of the test rig.For the narrow annular gap,there is an increase of non-dimensional tangential velocity V/Ωr with radial location to solid body rotation V/Ωr=1.For the wider annular gap,the non-dimensional velocities show a decrease with radial location to solid body rotation.      

Research on Auto-detection for Remainder Particles of Aerospace Relay Based on Wavelet Analysis

Aerospace relay is one kind of electronic components which is used widely in national defense system and aerospace system. The existence of remainder particles induces the reliability declining, which has become a severe problem in the development of aerospace relay. Traditional particle impact noise detection (PIND) method for remainder detection is ineffective for small particles, due to its low precision and involvement of subjective factors. An auto-detection method for PIND output signals is proposed in this paper, which is based on direct wavelet de-noising (DWD), cross-correlation analysis (CCA) and homo-filtering (HF), the method enhances the affectiv-ity of PIND test about the small particles. In the end, some practical PIND output signals are analysed, and the validity of this new method is proved.     

Preparation of Highly Dispersed Antimony-doped Tin Oxide Nano-powder via Ion-exchange Hydrolysis of SnCl4 and SbCl3 and Azeotropic Drying

Antimony-doped tin hydroxide colloid precipitates have been synthesized by hydrolysis of SnCl4 and SbCl3 using: (1) an ion-exchange hydrolysis to remove chlorine ions, and (2) isoamyl acetate as an azeotropic solvent to obviate water. The obtained dried powder is of high dispersivity without any need for further grinding. The size and dispersivity of the final particles are investigated with the aid of TG-DTA, BET, XRD and TEM. After having calcined, the antimony-doped tin oxide nanopowder possesses a tetragonal rutile structure with high dispersivity, uniform particles and low hard agglomeration.     

Effects of Mo on the Microstructure and Hydrogen Sorption Properties of Ti-Mo Getters

The effects of Mo on the microstructure evolution, porosity and hydrogen sorption properties of Ti-Mo getters are investigated in this work. The results show that the addition of Mo prolongs the densification process of Ti-Mo getters and results in a significant amount of sintered pores. With the Mo content increasing, the porosity of getters firstly increases reaching the maximum value as it at- tains about 7.5wt.%, and then drops. At the room temperature, the hydrogen sorption property of getters increases progressively with the Mo content increasing, but the tendency is not very clear before its content lies below 2.5wt.%. When the Mo content achieves about 7.5wt.%, the hydrogen sorption property proves to be the best. The discussion is made about the above mentioned phenomena inclusive of hydrogen sorption properties of getters under different activation conditions (from 500-750 ℃).     

超声速燃烧数值模拟中的湍流与化学反应相互作用模型

高精度数值模拟有助于理解超声速湍流燃烧中湍流与化学反应的相互作用,可为发动机燃烧室等工程应用设计提供可靠的预测模型。除直接数值模拟外,目前在湍流燃烧应用中使用的大涡模拟和雷诺平均Navier-Stokes模拟均需要借助模型模化发生在湍流小尺度上的流动与化学反应过程对湍流大尺度运动的影响。现有的湍流与化学反应相互作用模型大致可分为:火焰面类模型和概率密度函数类模型,2类模型在不同的应用中各自具有优势和局限性。此外,现有模型大都基于低马赫数燃烧,而超声速燃烧中通常会伴随快速混合、局部熄火和再着火以及激波等复杂过程,这为发展其中的湍流与化学反应相互作用模型提出了更多的挑战。     

适于低轨卫星IP网络的单核共享树组播算法(英文)

为了解决低轨卫星IP网络中现有典型源组播算法的信道资源浪费问题,本文提出了一套单核共享树组播算法,即核心群合并共享树(CCST)和加权核心群合并共享树(w-CCST)算法。CCST 算法包括动态近似中心(DAC)选核方法和核心群合并组播路径构建方法。DAC方法专为周期、规律运动的低轨卫星网络提出,不需要复杂的星上计算。在核心群合并方法中,以核节点作为初始核心群,通过核心群和剩余组成员的最短路径方法逐步扩展直至整棵组播树构建完成,从而使得组播树的树代价最小,大大提高了网络的带宽利用率和组播传输效率。w-CCST 算法中所提出的加权因子可以调整树代价和端到端传播时延之间的折衷程度,因此,可以通过调整加权因子来适度增大树代价、降低端到端传播时延以支持某些端到端时延要求苛刻的实时组播业务。最后,与低轨卫星 IP 网络中典型算法进行了性能比较,仿真结果说明,CCST 算法的平均树代价比其它算法显著降低,w-CCST 算法的平均端到端传播时延小于 CCST 算法。     

Jet Vectoring Control Using a Novel Synthetic Jet Actuator

A primary air jet vectoring control system with a novel synthetic jet actuator (SJA) is presented and simulated numerically. The results show that, in comparison with an existing traditional synthetic jet actuator, which is able to perform the duty of either “push” or “pull”, one novel synthetic jet actuator can fulfill both “push” and “pull” functions to vector the primary jet by shifting a slide block inside it. Therefore, because the new actuator possesses greater efficiency, it has potentiality to replace the existing one in various appli- cations, such as thrust vectoring and the reduction of thermal signature. Moreover, as the novel actuator can fulfill those functions that the existing one can not, it may well be expected to popularize it into more flow control systems.     

Nonlinear Adaptive Slewing Motion Control of Spacecraft Truss Driven by Synchronous V-gimbaled CMG Precession

The slewing motion control of a truss arm driven by a V-gimbaled control-moment-gyro (CMG) is a nonlinear control problem. The V-gimbaled CMG consists of a pair of gyros that must precess synchronously. The moment of inertia of the system, the angular momentum of the gyros and the external disturbances are not exactly known. With the help of feedback linearization and recursive Lyapunov design method, an adaptive nonlinear controller is designed to deal with the unknown items. Performance of the proposed controller is verified by simulation.     

An SOR Implicit Time-accurate Scheme in Calculating Unsteady Flows

A new time-accurate marching scheme for unsteady flow calculations is proposed in the present work. This method is the combination of classical Successive Over-Relaxation (SOR) iteration method and Jacobian matrix diagonally dominant splitting method of LUSGS. One advantage of this algorithm is the second-order accuracy because of no factorization error. Another advantage is the low computational cost because the Jacobian matrices and fluxes are only calculated once in each physical time step. And, the SOR algorithm has better convergence property than Gauss-Seidel. To investigate its accuracy and convergency, several unsteady flow computa- tional tests are carried out by using the proposed SOR algorithm. Roe’s FDS scheme is used to discritize the inviscid flux terms. Un- steady computational results of SOR are compared with the experiment results and those of Gauss-Seidel. Results reveal that the numerical results agree well with the experimental data and the second-order accuracy can be obtained as the Gauss-Seidel for unsteady flow computations. The impact of SOR factor is investigated for unsteady computations by using different SOR factors in this algorithm to simulate each computational test. Different numbers of inner iterations are needed to converge to the same criterion for different SOR factors and optimal choice of SOR factor can improve the computational efficiency greatly.