Flow field generated by a dielectric barrier discharge plasma actuator in quiescent air at initiation stage

A single Dielectric Barrier Discharge (DBD) plasma actuator driven by Alternating Current (AC) power, capable of inducing a starting vortex and a wall jet in quiescent air, is suited for low-Reynolds-number flow control. However, the starting vortex and the wall jet are usually observed after the plasma actuator has been operated for dozens of and hundreds of cycles of the voltage, respectively. The detail of the induced flow field at the initiation stage of the plasma actuator has rarely been addressed. At the initiation stage, a thin jet that provides the impetus for the entrainment of the induced flow at the beginning of the plasma actuation is first observed by using a high-accuracy phase-lock Schlieren technique and a high-speed Particle Image Velocimetry (PIV) system. This is the initial form of the momentum transfer from the plasma to the fluid. Then, an arched type jet is created by the plasma actuator. In addition, the whole development process of the induced flow field from the starting point of the thin jet to the quasi-steady stage of wall jet is presented for providing a comprehensive understanding of the plasma actuator and proposing a relevant enhancement of the numerical simulation model.     

一次火箭流量对RBCC性能影响的数值和实验研究

利用三维两相数值计算方法和地面直联试验系统,开展了不同来流速度下一次火箭流量变化对发动机性能的影响。数值研究结果表明,在不同来流条件下,一次流流量的增加对发动机推力和比冲的贡献不同,在低速条件时,一次火箭流量的增加对来流空气的加热以及缩短二次燃料的雾化蒸发时间和距离起着积极的作用,对性能的提高有一定作用;当来流速度较高时,过大一次流流量对流动通道产生了阻塞效应,造成对推力和比冲贡献作用的减小。试验结果验证了数值研究得到的规律,特别在高马赫数条件下,一次火箭流量的增加对推力和比冲的贡献是减小的,且飞行速度越高,这种贡献越小。无论低速还是高速来流条件,存在着一个优化的一次流流量,这对提高发动机性能有很大好处。     

喷气燃料热氧化安定性对航空发动机燃油系统沉积物生成的影响研究

利用HiReTS试验机[1]模拟发动机燃油系统,对喷气燃料沉积物的生成进行了研究。试验结果表明:加入自行研制的高热安定性添加剂,可有效提高喷气燃料的热氧化安定性;使用提高热氧化安定性的喷气燃料可以显著减少燃油系统沉积物的生成,从而延长发动机的使用寿命。     

气液针栓喷注单元雾化角模型

为了准确预测气液针栓喷注单元的雾化角,基于动量守恒建立了液束撞击气膜的雾化角理论模型,通过试验结果获得变形因子,并分析了结构参数和工况参数对雾化角的影响规律.结果表明:局部动量比对雾化角影响最大,其他结构参数和工况参数都是通过影响局部动量比而进一步决定雾化角;随着局部动量比增大,液束变形程度减小,液束变形导致有效撞击动...     

原子氧环境下磁力矩器用聚合物材料的质损和红外光谱分析

文章利用新型的原子氧环境模拟设备进行真空和原子氧试验,通过质量损失测量和FT-IR分析,对试样的质量损失率(SAML)和表面成分的变化进行了研究。试验结果表明:真空环境会导致材料产生质量损失,4种材料中真空质损最大相差24倍;原子氧作用导致聚合物材料产生质量损失,4种材料中质量损失率最大相差25倍;原子氧与有机硅物质反应能够形成保护层,可以抑制原子氧对材料内部的进一步侵蚀。FT-IR分析结果表明,原子氧作用导致环氧材料的-N消失,O元素百分比含量升高,硅橡胶的化学键被破坏,并导致新的O-H和C-H的生成。     

气膜冷却传热传质类比研究

应用SSTκ-ω湍流模型,对三维粘性掺混流场进行了数值模拟,得到了切向入射的超声速氢气膜在不同吹风比和被冷却面上的绝热温比分布,并通过冷却剂分布情况详细研究了其形成原因。计算结果表明：吹风比是决定超声速气膜冷却效果的重要因素,吹风比增大,冷却效果随之提高;不同曲率的曲面上,冷却效率的分布规律不同,凹面上冷却效果最好,这与低速气膜冷却不同;离散孔在被冷却面中心和两侧的冷却效果存在明显差异,引入一定的侧向倾角使这种差异趋向消失。     

Science objectives of the magnetic field experiment onboard Aditya-L1 spacecraft

The Aditya-L1 is first Indian solar mission scheduled to be placed in a halo orbit around the first Lagrangian point (L1) of Sun-Earth system in the year 2018–19. The approved scientific payloads onboard Aditya-L1 spacecraft includes a Fluxgate Digital Magnetometer (FGM) to measure the local magnetic field which is necessary to supplement the outcome of other scientific experiments onboard. The in-situ vector magnetic field data at L1 is essential for better understanding of the data provided by the particle and plasma analysis experiments, onboard Aditya-L1 mission. Also, the dynamics of Coronal Mass Ejections (CMEs) can be better understood with the help of in-situ magnetic field data at the L1 point region. This data will also serve as crucial input for the short lead-time space weather forecasting models.The proposed FGM is a dual range magnetic sensor on a 6?m long boom mounted on the Sun viewing panel deck and configured to deploy along the negative roll direction of the spacecraft. Two sets of sensors (tri-axial each) are proposed to be mounted, one at the tip of boom (6?m from the spacecraft) and other, midway (3?m from the spacecraft). The main science objective of this experiment is to measure the magnitude and nature of the interplanetary magnetic field (IMF) locally and to study the disturbed magnetic conditions and extreme solar events by detecting the CME from Sun as a transient event. The proposed secondary science objectives are to study the impact of interplanetary structures and shock solar wind interaction on geo-space environment and to detect low frequency plasma waves emanating from the solar corona at L1 point. This will provide a better understanding on how the Sun affects interplanetary space.In this paper, we shall give the main scientific objectives of the magnetic field experiment and brief technical details of the FGM onboard Aditya-1 spacecraft.     

充液航天器质量特性计算方法研究

充液航天器的质量特性对飞行动力学建模和控制设计有着重要影响。质量特性测量装置通常只能测出干重状态下航天器的质量特性，而充液状态下的航天器质量特性只能靠计算给出，其中如何计及各贮箱内液体的惯性张量是此类工程计算的难点。首先采用势流理论推导了任意形状贮箱内液体质量特性的一般表达式，包括全充液情况和部分充液情况，其中对部分充液情况考虑了自由液面小幅晃动的影响；然后采用三维有限元方法建立了液体质量特性的数值计算方法，并通过一个验证算例确认了该计算方法的有效性；最后应用该方法计算了一个充液航天器的质量特性，并研究了不同的液体处理方法对计算结果的影响。研究表明，工程上通常采用的“固化液体”处理方法所计算出来的转动惯量明显偏大，而所提出的计算方法具有更好的理论正确性和工程适用性。     

Analysis of a long-duration AR throughout five solar rotations: Magnetic properties and ejective events

Coronal mass ejections (CMEs), which are among the most magnificent solar eruptions, are a major driver of space weather and can thus affect diverse human technologies. Different processes have been proposed to explain the initiation and release of CMEs from solar active regions (ARs), without reaching consensus on which is the predominant scenario, and thus rendering impossible to accurately predict when a CME is going to erupt from a given AR. To investigate AR magnetic properties that favor CMEs production, we employ multi-spacecraft data to analyze a long duration AR (NOAA 11089, 11100, 11106, 11112 and 11121) throughout its complete lifetime, spanning five Carrington rotations from July to November 2010. We use data from the Solar Dynamics Observatory to study the evolution of the AR magnetic properties during the five near-side passages, and a proxy to follow the magnetic flux changes when no magnetograms are available, i.e. during far-side transits. The ejectivity is studied by characterizing the angular widths, speeds and masses of 108 CMEs that we associated to the AR, when examining a 124-day period. Such an ejectivity tracking was possible thanks to the multi-viewpoint images provided by the Solar-Terrestrial Relations Observatory and Solar and Heliospheric Observatory in a quasi-quadrature configuration. We also inspected the X-ray flares registered by the GOES satellite and found 162 to be associated to the AR under study. Given the substantial number of ejections studied, we use a statistical approach instead of a single-event analysis. We found three well defined periods of very high CMEs activity and two periods with no mass ejections that are preceded or accompanied by characteristic changes in the AR magnetic flux, free magnetic energy and/or presence of electric currents. Our large sample of CMEs and long term study of a single AR, provide further evidence relating AR magnetic activity to CME and Flare production.     

亚声速矩形射流的噪声辐射特性和声源分布

基于射流噪声模拟试验台，对出口面积相同的圆形喷口及宽高比分别为1、1.5、2、10的矩形喷口亚声速射流的远场噪声辐射特性和噪声源分布位置进行了较为系统的研究。通过远场噪声测量，获得了不同宽高比矩形喷口在不同方位角平面的射流噪声频谱分布结果相对于圆形射流的差异，揭示了矩形射流潜在的降噪潜力。通过基于波束成形算法的传声器阵列，得到了矩形射流噪声源峰值位置随频率的变化情况，系统分析了射流速度、方位角、宽高比等参数对矩形射流噪声源分布的影响。射流速度和方位角对矩形射流噪声源分布的归一化结果影响很小，而宽高比对矩形射流噪声源分布有较大影响：随着矩形宽高比的增加，矩形射流低频段噪声源向上游偏移，高频段噪声源向下游偏移。