一种引射增强型二次喉道新方案的数值模拟

为提高大型超声速风洞的运行经济性，设计了一种通过引射低总压冷介质提高扩压性能的新型二次喉道扩压器，其结构特征是在扩压器收敛段前方增加侧壁凹槽，在凹槽前沿位置引入低总压常温空气作为冷介质，通过引射扩散作用在扩压器壁面形成气膜，调节二次喉道实际流通直径，较大程度上增强二次喉道的静压恢复能力，同时又降低二次喉道壁面热负荷，冷却壁面。数值验证结果表明，所设计新型二次喉道方案可通过调节引射气量自适应较宽范围的运行条件，有效隔离扩压器壁面直接接触高温燃气，同时提高了扩压能力，节省后段接力引射器的主动流流量近30%，对风洞运行经济性提升十分明显。     

尖侧缘机身布局的俯仰力矩特性及扰流板控制

针对尖侧缘机身布局在大迎角下存在的正俯仰力矩（抬头力矩）问题，通过风洞试验，首先研究了俯仰力矩的迎角分区特性及流动演化规律：线性增长区（迎角为0°~15°），俯仰力矩线性增加，全机从附着流到形成进气道前缘涡和机翼涡；非线性增长区（迎角为17.5°~32.5°），俯仰力矩非线性增加，机头涡出现，机头涡和进气道前缘涡逐渐增强，机翼涡增强后破裂；衰减区（迎角为35°~65°），俯仰力矩逐渐减小，机头涡增强后破裂，进气道前缘涡破裂发展，机翼涡完全破裂。其次，发现了机身前体是产生正俯仰力矩的主要来源，机头涡是导致大迎角下正俯仰力矩的主控流动。当迎角为40°时，前体各截面正俯仰力矩在进气道前缘处达到最大，主要是由于该处机头涡诱导产生了较强的法向力。最后，提出了大迎角机身扰流板控制技术，产生了较好的控制效果。当迎角为40°时，扰流板可使正俯仰力矩减少62%，其原因是扰流板降低了机头涡涡量及其诱导产生的法向力，减少了机身前体对正俯仰力矩的贡献。该控制技术的缺点是扰流板会带来一些升力损失和附加阻力。基于尖侧缘机身参考宽度的雷诺数为2.59×10⁵。     

Effects of Mach numbers on Magnus induced surface pressure

Experimental and numerical methods were used to investigate the Magnus phenomena over a spinning projectile. The pressure force acting on the surface of a spinning projectile was measured for various cases by employing a relatively novel experimental technique. A set of miniature pressure sensors along with a data acquisition board, battery and storage memory were placed inside a spinning model and the surface pressure were obtained through a remotely controlled system. Circumferential pressures of the model for both rotational and static conditions were obtained at two different free stream Mach numbers of 0.4 and 0.8 and at different angles of attack. The results showed the ability of this new test method to measure the very small Magnus force via surface pressures over the projectile. The results provide a deep insight into the flow structure and illustrate changes in the cross-flow separation locations as a result of rotation. Similar results were obtained by the numerical simulations and were compared with the experimental data.     

全模颤振风洞试验三索悬挂系统多体动力学分析

全模颤振风洞试验需要通过软支撑系统模拟飞行器的自由飞行状态并调整模型姿态达到配平状态。参考NASA双索悬挂方案，提出了一种两电机驱动的三索悬挂系统，利用后方两索的同向/反向联动实现模型俯仰和滚转姿态的调整，利用弹簧刚度以及钢绳张力设计实现支撑频率要求。基于柔性多体动力学方法，建立了包括飞行器刚体模型、柔性索、滑轮、弹簧、气动力模型、伺服电机控制在内的复杂系统动力学模型，其中，利用任意拉格朗日-欧拉（ALE）变长度索单元描述钢绳，利用不约束物质坐标的索结点约束描述钢绳与滑轮相互作用，利用索结点物质输运速度约束描述伺服电机绞盘，利用飞行力学的气动力模型描述吹风下的气动力。基于该模型，通过小扰动响应辨识研究了弹簧刚度、钢绳张力、连接点位置等因素对支撑频率的影响规律，并分析了系统姿态调整能力，俯仰调整范围达到-12.5°~12.5°，滚转调整范围达到-45°~45°。采用滑轮处电位计测量的钢绳相对位移作为反馈信号，基于设计的控制律利用多体动力学求解器与Simulink对风洞吹风下的姿态调整过程进行仿真，模型达到配平状态，获得了吹风下的索拉力和伺服电机功率，为系统设计提供基础。     

某飞行器推力矢量试验测力装置研制

为满足某飞行器推力矢量试验的测试要求,采用两台六分量应变天平和一个空气桥组成测力装置来实现飞机全机气动力和喷管推进特性同时分别测量。基于有限元软件,对天平的应变及空气桥对天平的干扰进行了分析。结果表明:空气桥对天平力分量的干扰值优于5%,对力矩(滚转力矩除外)分量的干扰值优于15%,达到了设计指标。通过校准获得了单独天平、天平带空气桥(充压、不充压)状态下的校准公式,校准结果表明:两台天平各分量的综合加载误差均优于0.3%,天平带空气桥(充压、不充压)状态下各分量的综合加载误差优于0.5%,空气桥对天平的干扰量值与有限元分析结果一致。理论分析与实测结果证明:研制的天平及空气桥达到了预定目标,它的测量精准度高,满足推力矢量风洞试验需求。     

Remote-controlled flexible pose measurement system and method for a moving target in wind tunnel

The measurement of position and attitude parameters for the isolated target from a high-speed aircraft is a great challenge in the field of wind tunnel simulation technology. This paper proposes a remote-controlled flexible pose measurement system in wind tunnel conditions for the separation of a target from an aircraft. The position and attitude parameters of a moving object are obtained by utilizing a single camera with a focal length and camera orientation that can be changed based on different measurement conditions. Using this proposed system and method, both the flexibility and efficiency of the pose measurement system can be enhanced in wind tunnel conditions to meet the measurement requirements of different objects and experiments, which is also useful for the development of an intelligent position and attitude measurement system. The position and the focal length of the camera also can be controlled remotely during measurements to enlarge both the vertical and horizontal measurement range of this system. Experiments are conducted in the laboratory to measure the position and attitude of moving objects with high flexibility and efficiency, and the measurement precision of the measurement system is also verified through experiments.     

27-day variation in solar-terrestrial parameters: Global characteristics and an origin based approach of the signals

The Earth and the near interplanetary medium are affected by the Sun in different ways. Those processes generated in the Sun that induce perturbations into the Magnetosphere-Ionosphere system are called geoeffective processes and show a wide range of temporal variations, like the 11-year solar cycle (long term variations), the variation of ～27?days (recurrent variations), solar storms enduring for some days, particle acceleration events lasting for some hours, etc.In this article, the periodicity of ～27?days associated with the solar synodic rotation period is investigated. The work is mainly focused on studying the resulting 27-day periodic signal in the magnetic activity, by the analysis of the horizontal component of the magnetic field registered on a set of 103 magnetic observatories distributed around the world. For this a new method to isolate the periodicity of interest has been developed consisting of two main steps: the first one consists of removing the linear trend corresponding to every calendar year from the data series, and the second one of removing from the resulting series a smoothed version of it obtained by applying a 30-day moving average. The result at the end of this process is a data series in which all the signal with periods larger than 30?days are canceled.The most important characteristics observed in the resulting signals are two main amplitude modulations: the first and most prominent related to the 11-year solar cycle and the second one with a semiannual pattern. In addition, the amplitude of the signal shows a dependence on the geomagnetic latitude of the observatory with a significant discontinuity at approx. ±60°.The processing scheme was also applied to other parameters that are widely used to characterize the energy transfer from the Sun to the Earth: F10.7 and Mg II indices and the ionospheric vertical total electron content (vTEC) were considered for radiative interactions; and the solar wind velocity for the non-radiative interactions between the solar wind and the magnetosphere. The 27-day signal obtained in the magnetic activity was compared with the signals found in the other parameters resulting in a series of cross-correlations curves with maximum correlation between 3 and 5?days of delays for the radiative and between 0 and 1?days of delay for the non-radiative parameters. This result supports the idea that the physical process responsible for the 27-day signal in the magnetic activity is related to the solar wind and not to the solar electromagnetic radiation.     

Variation of dayside chorus waves associated with solar wind dynamic pressure based on MMS observations

The whistler-mode chorus waves are one of the most important plasma waves in the Earth’s magnetosphere. Generally, the amplitude of whistler-mode chorus waves prefers to strengthen when the energetic fluxes of anisotropic electrons increase outside the plasmapause. This characteristic is commonly associated with the geomagnetic storms or substorms. However, the relationship between the solar wind dynamic pressure (P_sw) and the long-time variation of chorus waves during the quiet period of the geomagnetic activity still needs more detailed investigations. In this paper, based on MMS observations, we present a chorus event just observed in the inner side of magnetopause without obvious geomagnetic storms or substroms. Interestingly, during this time interval, some P_sw fluctuations were recorded. Both the amplitudes and frequencies of chorus waves changed as a response to the variation in P_sw. It proved that the enhancement of P_sw increases the energetic electrons fluxes, which provides free energies for the chorus amplification. Furthermore, the wave growth rates calculated using linear theory increases and the central frequency of the chorus waves shifts to a higher frequency when the P_sw enhancement is greater, which are also consistent well with the observations. The results provide a direct evidence that the P_sw play an important role in the long-time variation of whistler-mode chorus waves inside the magnetopause.     

0.3 m低温风洞液氮供给系统研制

基于系统级的一维热流体模拟分析,建立了适用于研究分析0.3 m低温风洞液氮供给系统的数学模型,并开展了系统漏热、两相流及缓冲罐中液氮容积等流体动力学分析;在系统现有控制策略及试验数据的基础上,基于该数学模型开展了系统压力动态响应分析,获得了在阀门动态调节过程中管网压力的瞬态响应,计算结果与试验值的总体误差控制在10%以内。喷射压力一致化改造避免了阀间干扰,添加的回流管道消除了供给末端的两相流现象,使喷射压力控制精度达到1.1%,调节时间减少到23 s,实现了风洞总温快速安全调节和精确控制。     

基于激光多普勒原理的极低风速测量实验

介绍了利用激光多普勒效应进行风速测量的原理及定点遥测原理,分析了探测气溶胶颗粒大小的要求,并以此搭建了一套极低风速测量系统。同时分析了系统的测速精度,以及安装角度对测量结果的影响。最后分别开展了转台实验、直线导轨实验和风洞实验,实验结果表明,该极低风速测量系统的测量误差基本可以控制在001 m/s以内,当风洞工作介质为未经处理的环境空气时,系统可以获得稳定可靠的信号,测量结果与高性能仪器十分接近。