高超声速飞行器发动机热防护与发电一体化系统

在对高超声速飞行器的热防护和机载设备电能需求的综合考虑下,立足发动机能量管理优化,结合CO2的物性特点,提出了以超临界CO2为循环工质的高效热防护与高温发电一体化系统.此一体化方案可以在实现发动机热防护的同时,提供电能、并减少冷却用燃油流量.基于燃油为该一体化系统的唯一热沉,通过理论分析和计算,提出了两个一体化系统,通...     

半开式富氧补燃混合循环发动机方案研究

针对未来航天主发动机的应用需求,提出了一种燃料供应系统采用开式循环、氧化剂供应系统采用分级燃烧闭式循环的半开式富氧补燃混合循环发动机系统方案,综合分析了这种新型混合循环发动机所能达到的比冲性能,对比分析了新型混合循环发动机作为可重复使用航天运载器主发动机相比于开式循环和常规补燃循环、全流量补燃循环发动机的优缺点,针对推...     

基于3维数值仿真的变循环压缩系统部件匹配分析

为了研究变循环压缩系统中各部件之间的匹配关系以及在整机调节时的表现,采用3维数值仿真软件对变循环发动机 的风扇、核心机驱动风扇级（CDFS）、高压压气机和外涵道开展联合数值仿真,并对比数值计算与试验结果的差异。针对单、双涵 工作模式,开展内、外涵出口节流特性计算,分析了内、外涵出口压力调节导致的各部件匹配关系的变化,获得了涵道比的变化范 围以及极限调节状态下的各部件表现出的流动特征,确定了制约整个压缩系统喘振裕度的关键部件。结果表明：在双涵模式下, 外涵节流导致风扇匹配点明显提高,首先到达喘振边界;在单涵模式下,外涵节流导致风扇和CDFS匹配点同时提高,几乎同时到 达喘振边界;在单、双涵模式下,内涵节流均使高压压气机首先到达喘振边界。仿真得到的外涵道损失与试验偏差在4%以内。     

细长三角翼摇滚运动数值研究

采用亚迭代耦合求解流体动力学方程和刚体动力学方程数值研究方法,建立流体与刚体运动耦合的无时间滞后的数值手段来分析研究飞行器非定常的耦合运动特征,预测失稳运动的发生与发展。研究表明:在流动结构失稳后机体运动逐步形成极限环振荡的周期性自维持运动,滚转力矩系数滞回曲线呈现典型的”双8”稳定形态,前缘涡的非对称飘起与再附是典型三角翼摇滚的驱动形式;三角翼构型的自由滚振幅随攻角变化呈现阶跃式的变化;自激振荡的幅度及频率与滚动惯量的大小存在对应的规律性关系。非定常自激振动的翼摇滚具有多控制参数、非稳定、非线性的运动特征。     

全动翼面间隙非线性气动弹性响应分析

战斗机全动翼面操纵系统中普遍存在间隙,其非线性特性不但影响系统地面振动试验数据的有效性,而且可能导致飞行器气动弹性稳定性边界产生偏差,因此有必要开展考虑间隙非线性的气动弹性响应分析研究。以全动翼面旋转方向间隙为研究对象,基于虚拟质量法线性化模态振型,建立一组可以表达整个响应域变形的统一模态振型;采用有理函数拟合,将频域非定常气动力转换到时域,分析不同间隙参数对应的极限环响应特性。结果表明：当全动翼面结构系统中存在间隙时,在低于线性颤振边界的特定飞行区域,翼面会出现非线性极限环振荡现象,间隙参数会影响极限环振荡幅值、频率以及极限环振荡的进入临界速压和发散临界速压。     

Analysis of ionospheric TEC response to solar and geomagnetic activities at different solar activity stages

Studying the relationship of total electron content (TEC) to solar or geomagnetic activities at different solar activity stages can provide a reference for ionospheric modeling and prediction. On the basis of solar activity indices, geomagnetic activity parameters, and ionospheric TEC data at different solar activity stages, this study analyzes the overall variation relationships of solar and geomagnetic activities with ionospheric TEC, the characteristics of the quasi-27-day periodic oscillations of the three variables at different stages, and the delayed TEC response of solar activity by conducting correlation analysis, Butterworth band-pass filtering, Fourier transform, and time lag analysis. The following results are obtained. (1) TEC exhibits a significant linear relationship with solar activity at different solar activity stages. The correlation coefficients |R| are arranged as follows: |R|_EUV > |R|_F10.7 > |R|sunspot number. No significant linear relationship exists between TEC and geomagnetic activity parameters (|R| < 0.35). (2) TEC, solar activity indices, and geomagnetic activity parameters have a period of 10.5 years. The maximum amplitudes of the Fourier spectrum for TEC and solar activity indices are nearly 27 days and those of geomagnetic activity parameters are nearly 27 and 13.5 days. (3) The deviations of the quasi-27-day significant periodic oscillation of TEC and solar activity indices are consistent. (4) No evident relationship exists between the quasi-27-day periodic oscillation of TEC and geomagnetic activity parameters. (5) The delay time of TEC for the 10.7 cm solar radio flux and extreme ultraviolet is always consistent, whereas that for sunspot number varies at each stage.     

预冷组合循环发动机吸气式模态建模与性能分析

为了对预冷组合循环发动机开展性能分析，以协同吸气式火箭发动机（SABRE 4）为研究对象，采用部件法建立了发动机稳态模型，计算获得了SABRE 4发动机在吸气式模态下沿飞行弹道的性能参数变化规律。然后对发动机的高度和速度特性进行研究，得到了发动机的飞行包线。计算结果表明，在吸气式飞行弹道内，核心机推力和比冲的变化分别为488~680kN和34786~46954m/s。SABRE 4发动机具备推力大和比冲高的性能优势。在预冷器工作过程中，随着飞行马赫数增大，预冷器换热量不断增大，进入预燃室的氢流量减小，预燃室总温降低，HX3的吸热量减小。与其他压气机和涡轮相比，空气压气机和氦涡轮的工作参数变化较大。SABRE 4发动机通过对来流空气进行预冷，可实现在大空域和宽速域内工作。由于空气压气机的喘振和堵塞边界限制，发动机的高度和速度特性分别存在飞行高度和飞行马赫数的限制。     

兆瓦级空间核电源碱金属朗肯循环热电转换系统设计

为解决火星探测任务中存在的星表供电问题,制定了以空间液态金属朗肯循环作为星表基地热电转换模块的任务规划,采用Simulink模块化建模方法对空间液态金属朗肯循环模型进行程序化描述.根据空间朗肯循环各部件的耦合标准,建立系统部件及总体控制仿真模型,重点研究变运行条件下循环输出功率的波动.研究表明:在本文各工况下,朗肯循环...     

A model of foreground emission in UV using GALEX deep observations

Foreground emission, mainly airglow and zodiacal light, is a significant contributor in an ultraviolet observation especially from low earth orbit. Its careful estimation and removal are tedious yet unavoidable processes in the study of diffuse UV radiation and by extension interstellar dust studies. Our analysis of deep GALEX observations show that airglow is not only a function of Sun angle but also a strong function of Solar activity at the time of observation. We present here an empirical model of airglow emission, derived from GALEX deep observations, as a function of 10.7 cm Solar flux and Sun angle. We obtained the model by training machine learning models on the data using a variant of the regression algorithm that is both resilient toward outlier data and sensitive to the complexities of the provided data. Our model predictions across various observations show no loss in generalization as well as good agreement with the observed values. We find that the total airglow in an observation is the sum of a baseline part (AG_c) that depends on the Solar flux and Sun angle, and a variable part (AG_v) that depends on the Sun angle and the time of observation with respect to local midnight. We also find that the total airglow can vary between 85 – 390 photon units in FUV and 80 – 465 photon units in NUV.     

Investigations of entrainment characteristics and shear-layer vortices evolution in an axisymmetric rear variable area bypass injector

In this study,firstly,for the axisymmetric RVABI,the change-rule of adverse pressure gradient caused by radial velocity during the transition of internal flow mode in variable geometry is summarized,and a Bypass Ratio(BR) iterative algorithm based on the empirical correlation of non-equilibrium pressure is proposed.The algorithm can estimate the nonlinear relationship between area ratio and BR,with an error range falling below 6.5%.Then,we discuss the favorable effect of uniform mixing on the th...