涡轮叶冠换热特性实验与数值模拟

利用数值模拟及实验方法对涡轮叶冠间隙流场换热特性进行了研究,分析静止状态下叶尖泄漏流雷诺数、前后孔岀流比、叶尖间隙等参数对叶冠的表面传热系数的影响.结果表明:叶冠转速的变化对表面传热系数影响较小;随着泄漏流雷诺数的增加,叶冠的平均表面传热系数增大;平均表面传热系数随前、后孔岀流比增大而增大,其中前孔出流比的影响较为明显;叶尖间隙减小,平均表面传热系数增大,并且随叶尖间隙的减小,增长越来越快.将计算与实验结果进行了比较,吻合良好,误差小于10%.      

基于涡格法的近程无人机气动优化与风洞实验验证

针对低雷诺数的近程无人机,利用涡格法（VLM）对无人机气动特性进行了加装翼尖小翼优化设计,并通过风洞实验进行了验证。首先给出了翼尖小翼的几何参数并分析其对全机气动特性的影响,其次利用涡格法对小翼进行气动建模和优选,针对无人机巡航状态给出了小翼优化结果,最后利用风洞实验对优化前后的无人机进行了吹风实验对比验证,实验结果表明,涡格法和风洞实验结果在线性段相符,涡格法能够较准确地描述和预测翼尖小翼特性,加装翼尖小翼后的无人机巡航状态升阻比提高12％,全机滚转阻尼加大,偏航阻尼变化很小。     

某运输机全机构型雷诺数效应阻力修正研究

采用CFD方法分析了雷诺数效应对某运输机全机构型阻力的影响。基于对某运输机的翼/身/架/舱组合体绕流进行的计算分析,归纳总结出了一种适应于复杂构型的低雷诺数到高雷诺数的阻力修正方法。通过验证可知,该修正方法修正效果良好,为工程中的阻力预测提供了一种简洁有效的方法。     

Linkage of the ionospheric peak electron density and height deduced from the topside sounding data

Topside sounding electron density profiles are analyzed to explore interrelations of the F2 layer critical frequency and the peak height for a representative set of conditions provided by ISIS1, ISIS2, IK19 and Cosmos-1809 satellites for the period of 1969–1987. The foF2 and hmF2 are delivered with exponential extrapolation of electron density profile to zero of its 1st derivative. It is shown that the linear regression exists between foF2 and hmF2 under different conditions. The linkage between the two parameters amended to the empirical model of the peak height [Gulyaeva, T.L., Bradley, P.A., Stanislawska, I., Juchnikowski, G. Towards a new reference model of hmF2 for IRI. Adv. Space Res. 42, 666–672, doi:10.1016/j.asr.2008.02.021, 2008] results in an empirical model of the both foF2 and hmF2 expressed by superposition of functions in terms of local-time, season, geodetic longitude, modified dip latitude and solar activity. For the solar activity we use a proxy Fsp index averaged from the mean solar radio flux F10.7s for the past 81 days (3 solar rotations) and F10.7 value for 1 day prior the day of observation. Impact of geomagnetic activity is not discernible with the topside sounding data due to mixed positive and negative storm-time effects. Appreciable differences have been revealed between IRI-CCIR predictions and outcome of the new model which might be attributed to the different techniques of the peak electron density and height derivation, different epochs and different global distribution of the source data as well as the different mathematical functions involved in the maps and the model presentation.     

某涡轮级三维流场非定常数值研究

基于耦合Lantry-Menter转捩模型的SST(Shear stress transport)湍流模型,对某涡轮级在3个雷诺数工况下的全三维流场分别进行了定常、非定常数值模拟,目的在于对比分析两种计算方法所得结果之间的差异。计算结果表明,进口雷诺数为4×104时和5×105时,定常与非定常计算的涡轮级效率的差异较大,最大相差0.6个百分点,而当雷诺数为8×104时,两者差异很小;非定常计算能够较好的模拟叶尖泄漏涡的发展过程、低雷诺数下上游尾迹与下游转子叶片吸力面分离边界层干涉诱导卷起涡的形成、输运及其所导致的叶片吸力面表面压力大幅波动等非定常流动现象。最后,给出了转子出口截面上周向与径向的非定常压力脉动的分布,为基于Lighthill声类比方法的计算气动声学研究奠定了基础。     

扰流板进气总压畸变试验

在吊舱进气道进口安装扰流板进行试验,研究扰流板进气畸变的影响因素及总压畸变特征。试验得到了进气道出口若干马赫数下进气总压畸变的定量数据,研究了进气道出口压力分布和畸变指数随飞行马赫数、扰流板堵塞比、进气道出口马赫数的变化关系。试验结果表明：进气道出口对应点总压恢复系数随扰流板堵塞比和进气道出口马赫数的减小而增大,几乎不随飞行马赫数发生变化;受扰流板、飞行侧滑角以及发动机低压转子转向影响,进气道出口局部区域存在高压区,高压区域的大小和位置随飞行马赫数、扰流板堵塞比、进气道出口马赫数的变化而变化;各总压畸变指数随扰流板堵塞比和进气道出口马赫数增大而增大,飞行马赫数对畸变指数影响很小。同时,数值计算了不同飞行马赫数下进气道出口总压畸变特征及周向稳态畸变指数,与试验结果结论一致,验证了试验结果的可靠性,也证明了数值计算在总压畸变研究中的有效性。研究工作为进一步的空中逼喘试验奠定了基础。     

基于矩阵奇异值理论的颤振分析新方法

根据颤振分析的基本概念,提出了一类基于矩阵奇异值理论的颤振分析新方法。该方法的特点是,以计算颤振矩阵最小奇异值或条件数的倒数来直接搜索颤振临界点。证明了这两个指标在颤振临界点处的等价性。根据指标在颤振临界点附近取极小值的特点,编制了相应的算法,在确定颤振临界点时无需计算颤振特征根,避免了“窜支”问题,从而减少了人工干预,提高了计算自动化程度。数值算例结果表明,采用该方法计算得到的颤振临界速度和颤振频率与p-k法计算结果的精度相当,且两个指标对应的计算结果一致,验证了其等价性。     

强信号背景下弱信号角度时延的联合Capon估计方法

针对强信号背景下弱信号角度时延联合估计过程中的弱信号数目难以精确估计问题,在分析Capon谱估计法估计信号DOA原理的基础上,将Capon谱估计法进行扩展,提出了一种在强信号背景下弱信号角度时延联合估计方法。为弥补Capon法分辨力较差的劣势,将扩展的Capon法与有高分辨性能的m-Capon算法结合,提出了一种改进的m-Capon方法,能区分来波方向接近的不同目标信号。研究和仿真结果表明:该方法无需对弱信号的信源数进行估计,也无需分解特征值,且在快拍数较少时仍具适用性。     

Novel orbits of Mercury,Venus and Mars enabled using low-thrust propulsion

Exploration of the inner planets of the Solar System is vital to significantly enhance the understanding of the formulation of the Earth and other planets. This paper therefore considers the development of novel orbits of Mars, Mercury and Venus to enhance the opportunities for remote sensing of these planets. Continuous acceleration is used to extend the critical inclination of highly elliptical orbits at each planet and is shown to require modest thrust magnitudes. This paper also presents the extension of existing sun-synchronous orbits around Mars. However, unlike Earth and Mars, natural sun-synchronous orbits do not exist at Mercury or Venus. This research therefore also uses continuous acceleration to enable circular and elliptical sun-synchronous orbits, by ensuring that the orbit's nodal precession rate matches the planets mean orbital rate around the Sun, such that the lighting along the ground-track remains approximately constant over the mission duration. This property is useful both in terms of spacecraft design, due to the constant thermal conditions, and for comparison of images. Considerably high thrust levels are however required to enable these orbits, which are prohibitively high for orbits with inclinations around 90°. These orbits therefore require some development in electric propulsion systems before becoming feasible.