新型无尾联接翼布局气动特性研究

提出一种上下错开的无尾联接翼,即前翼或者后翼上反一定角度,使得前后翼垂直方向的相对距离从翼根处开始到翼梢处逐渐增大,以达到减小前后翼气动干扰的目的,搭接的小翼具有翼梢小翼作用,可有效减小诱导阻力。采用基于RANS方程的数值方法,研究了前后翼分别上反10°,20°和30°时对总体气动特性的影响,结果表明,当前翼上反且上反角为30°时其联接翼系统气动性能最佳。对该联接翼布局在Ma=0.85,0.95和1.20下进行了数值分析,结果表明,其升力系数变化较小,阻力系数在Ma0.85后才急剧增大,有应用于未来跨声速/超声速客机布局的潜力。     

飞行数据相容性检验方法

飞行试验测量数据中存在过程噪声和测量噪声,导致飞行数据之间不相容,国内目前常用的输出误差法不适用于耦合严重的直升机飞行数据相容性检验。采用增广卡尔曼滤波方法进行状态估计,大幅度地消除测量值中的误差;再用输出误差法对增广卡尔曼滤波估计的结果进行相容性检验,并将其应用于直升机四阶纵向等效模型辨识中。结果表明:提出的这种方法既解决了单独使用增广卡尔曼滤波进行数据相容性分析时由于初期收敛过程造成的滤波误差问题,又克服了单独使用输入误差法进行数据相容性时需手动修改时间延迟问题和测量值中误差过大时输出误差法无法收敛问题,使得检验效果与计算效率大幅提升。     

弹性空腔流致噪声/结构振动特性试验

高速空腔中经常存在高强度且多频率分量的流致噪声,空腔噪声与结构振动之间耦合效应严重,甚至可能发生结构共振。为此,在0.6m×0.6m高速风洞中,通过调整空腔底板厚度,改变其结构固有频率,模拟空腔流致噪声/振动相互作用。利用脉动压力和振动加速度测试技术,获取亚跨声速条件下,弹性空腔流致噪声特性及其结构振动响应特性。马赫数变化范围为0.6~1.2。结果表明,当振动强度较弱时,结构振动对空腔噪声影响较小,而空腔噪声对结构振动影响较大,在噪声载荷主频位置,振动谱出现峰值并且噪声/振动相关性达到最强;此外,空腔结构振动还与其固有频率特性密切相关,振动主要以低阶模态为主。     

基于人机闭环稳定性的舵机速率限制边界

舵机速率限制是造成电传操纵飞机人机耦合的主要原因。利用描述函数法对舵机速率限制非线性进行建模,分析舵机速率限制非线性、人机耦合发生频率及人机闭环稳定性间的关系,并基于此提出舵机速率边界的确定方法;以典型放宽静稳定性飞机为例,基于最优McRuer驾驶员模型,确定人机闭环稳定性所需的最小舵机偏转速率;基于开环起始点(OLOP)准则对所确定的速率限制边界进行验证。结果表明:本文提出的舵机速率边界的确定方法最小成本地避免了人机耦合;所确定的舵机速率限制边界与OLOP准则边界对应的舵机速率基本吻合,即所建立的舵机速率限制边界确定方法合理。     

颗粒无序分布的堆积床内部流动与传热分析

为了详细分析单组元发动机催化床内部的流动与传热,针对颗粒无序分布的堆积床,提出了一种网格生成途径,适合于对大量颗粒自然堆积的管道流动进行数值模拟。根据该方法,对不同颗粒直径、不同进口速度的管道堆积床进行了液体介质的流动与非定常传热模拟,并与实验结果和Ergun方程计算进行了对比。结果表明,本文提出的方法可以有效模拟颗粒无序分布的堆积床内部流动与传热,适合于大量颗粒的堆积床仿真;网格尺度小于1/20颗粒直径时,模拟结果与实验结果符合很好;在相同雷诺数下,摩擦系数随颗粒直径增大而减小,Ergun方程在高雷诺数下计算的流阻偏大;非定常传热时,壁面效应会使壁面附近温度先接近流体温度。     

Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals

Both heliophysics and planetary physics seek to understand the complex nature of the solar wind’s interaction with solar system obstacles like Earth’s magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle observations, guided by the predictions of both local and global numerical simulations, and placed in context by observations from far and extreme ultraviolet (FUV, EUV), hard X-ray, and energetic neutral atom imagers (ENA). Each proposed interaction mechanism (e.g., steady or transient magnetic reconnection, local or global magnetic reconnection, ion pick-up, or the Kelvin-Helmholtz instability) generates diagnostic plasma density structures. The significance of each mechanism to the overall interaction (as measured in terms of atmospheric/ionospheric loss at comets, Venus, and Mars or global magnetospheric/ionospheric convection at Earth) remains to be determined but can be evaluated on the basis of how often the density signatures that it generates are observed as a function of solar wind conditions. This paper reviews efforts to image the diagnostic plasma density structures in the soft (low energy, 0.1–2.0 keV) X-rays produced when high charge state solar wind ions exchange electrons with the exospheric neutrals surrounding solar system obstacles.The introduction notes that theory, local, and global simulations predict the characteristics of plasma boundaries such the bow shock and magnetopause (including location, density gradient, and motion) and regions such as the magnetosheath (including density and width) as a function of location, solar wind conditions, and the particular mechanism operating. In situ measurements confirm the existence of time- and spatial-dependent plasma density structures like the bow shock, magnetosheath, and magnetopause/ionopause at Venus, Mars, comets, and the Earth. However, in situ measurements rarely suffice to determine the global extent of these density structures or their global variation as a function of solar wind conditions, except in the form of empirical studies based on observations from many different times and solar wind conditions. Remote sensing observations provide global information about auroral ovals (FUV and hard X-ray), the terrestrial plasmasphere (EUV), and the terrestrial ring current (ENA). ENA instruments with low energy thresholds (\(\sim1~\mbox{keV}\)) have recently been used to obtain important information concerning the magnetosheaths of Venus, Mars, and the Earth. Recent technological developments make these magnetosheaths valuable potential targets for high-cadence wide-field-of-view soft X-ray imagers.Section 2 describes proposed dayside interaction mechanisms, including reconnection, the Kelvin-Helmholtz instability, and other processes in greater detail with an emphasis on the plasma density structures that they generate. It focuses upon the questions that remain as yet unanswered, such as the significance of each proposed interaction mode, which can be determined from its occurrence pattern as a function of location and solar wind conditions. Section 3 outlines the physics underlying the charge exchange generation of soft X-rays. Section 4 lists the background sources (helium focusing cone, planetary, and cosmic) of soft X-rays from which the charge exchange emissions generated by solar wind exchange must be distinguished. With the help of simulations employing state-of-the-art magnetohydrodynamic models for the solar wind-magnetosphere interaction, models for Earth’s exosphere, and knowledge concerning these background emissions, Sect. 5 demonstrates that boundaries and regions such as the bow shock, magnetosheath, magnetopause, and cusps can readily be identified in images of charge exchange emissions. Section 6 reviews observations by (generally narrow) field of view (FOV) astrophysical telescopes that confirm the presence of these emissions at the intensities predicted by the simulations. Section 7 describes the design of a notional wide FOV “lobster-eye” telescope capable of imaging the global interactions and shows how it might be used to extract information concerning the global interaction of the solar wind with solar system obstacles. The conclusion outlines prospects for missions employing such wide FOV imagers.     

非轴对称端壁设计的高负荷涡轮气热性能研究进展

非轴对称端壁设计因能够有效地减少涡轮叶栅的二次流损失和提高气动性能而在高负荷涡轮设计中得到应用。简要回顾了涡轮叶栅二次流模型和非轴对称端壁造型方法,重点综述了非轴对称端壁设计的高负荷涡轮气动性能研究进展和抑制端壁二次流的作用机制,介绍了非轴对称端壁设计的高负荷涡轮端壁气热耦合作用的冷却特性研究进展,总结了高负荷涡轮非轴对称端壁设计技术的应用成果,展望了非轴对称端壁设计在高负荷涡轮的高效气动和冷却布局应用方面需要深入研究的内容。     

嵌入式大气数据传感系统研究进展

大气数据的精确测量对飞行器的导航与控制至关重要。相较于传统的探针式大气数据测量系统,嵌入式大气数据传感系统更适用于隐身性能要求、大迎角飞行要求的飞行器或高超声速飞行器。回顾了嵌入式大气数据传感系统的发展历程,介绍了该系统完整的组成部分及其工作原理,并指出该系统在应用时的四项关键技术(测压孔布局、气动模型及求解算法、校正算法、故障检测及管理技术),结合国外多种飞行器上该系统不同的应用方案,分别对比分析四项关键技术不同应用方式的优缺点;指出了该系统的四项关键技术均会影响系统精度及可靠性,实际应用中需综合考虑选择其应用方式;最后展望了该系统在未来航空航天领域的应用。     

化学非平衡流动解耦算法的回顾与新进展

超声速化学非平衡流动的数值模拟一直是计算流体力学领域的难点,主要体现在如下几个方面：物理过程非常复杂,存在着激波、燃烧波等各种复杂波系的相互作用;超声速化学非平衡流动属于典型的时空多尺度物理问题,其控制方程存在严重的刚性,给数值求解带来了很大困难。对国内外的解耦算法研究现状简单综述后,主要介绍1993年刘君提出的解耦算法的理论基础,流动方程采用冻结流模型,源项方程模拟流体微团在当地绝热、定容的热力学系统内发生的化学反应过程。通过引入两个中间变量,即等效内能和等效比热比,将与温度无关的生成焓从流动方程组能量项中分离出去,源项方程组中包含等效内能,使用不同算子对流动方程和源项方程解耦求解。与传统解耦算法相比,源项方程的求解过程中包含状态参数和组元同时变化。结合刘君解耦算法机理和有限体积法空间平均特性,介绍近期在提高算法计算效率方面的研究进展,包括流动方程优化算法和耦合过程优化。采用优化算法对经典的激波诱导燃烧算例进行数值模拟,与不同文献结果进行对比,验证了优化算法的时空精度。通过总结经验发现化学非平衡反应仅发生在流场局部区域,提出质量生成率判据,结合相应模拟结果验证了方法的可行性,可以进一步提高化学反应算子的计算效率。     

叶轮行波振动下的气动阻尼计算

为展开运动边界下离心叶轮流场的数值分析,独立开发了网格变形程序和非定常流动模拟程序,实现了流场中振动离心叶轮的气动阻尼计算。采用紧支径向基函数法进行结构到气动表面变形的数据传递,应用二叉树技术进行壁面距离的计算,大幅提高了网格变形和流场分析中距离搜索的计算效率。通过振动叶栅和径向叶轮的算例,验证了程序应用于运动边界流场计算和叶轮流场模拟的正确性。以半开式叶轮为对象,展开其在行波振动条件下气动阻尼的计算分析。结果表明,叶轮在前、后行波振动下的气动阻尼均为正,后行波振动引起的气动推力和气动阻尼较大,叶轮表面的平均气动功率密度呈现循环对称的分布特征。