压电致动器扑翼结构动力学仿真

采用传统扑动机构的微型扑翼,气动效率低、扑动能耗大。采用压电致动器的微型扑翼通过压电材料进行致动使机翼产生上下扑动,有效地将扑动机构和机翼两个主要系统进行集成,不仅节省重量,同时它具有任务变形自适应能力强、气动效率高和扑动能耗小的特点。通过PCL语言建立采用压电致动器的扑翼有限元模型,结合同尺寸扑翼气动力试验数据,进行采用压电致动器扑翼结构仿真。利用仿真结果研制采用压电致动器扑翼原理样机,研究表明,采用压电致动器后扑翼扑动频率得到明显提高,压电片可有效控制机翼的弯扭变形,有助于提高扑翼的气动效率。     

基于参数化分析的柔性后缘优化设计

介绍了一种自适应柔性机翼后缘变形控制优化设计方法,该方法采用了由单个驱动器驱动的单块式分布柔性结构。该方法的关键在于设计一种合适的柔性后缘结构拓扑形式,使该自适应柔性机翼后缘能够达到精确的变形。阐明了柔性结构拓扑优化设计的数学模型,针对自适应柔性机翼后缘概念设计提出了基于参数化分析的拓扑优化设计方案,并进行了工程化圆整和尺寸优化。最终,通过非线性有限元分析和功能测试,验证了本文提出的柔性后缘优化设计方法的合理性。     

便携式充电设备检测系统的研究与设计

为了便于充电设备现场检测工作,设计了一种便携式直流充电设备现场检测系统。该系统功能具有完善的测试功能,能够方便的对直流充电设备进行检验测试,完全满足直流充电设备运行检测的需求。该系统具有小型化、便携化的优点,有利于提高现场检测效率,保证了充电设备运行的安全性及稳定性。     

OSIRIS-REx: Sample Return from Asteroid (101955) Bennu

In May of 2011, NASA selected the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) asteroid sample return mission as the third mission in the New Frontiers program. The other two New Frontiers missions are New Horizons, which explored Pluto during a flyby in July 2015 and is on its way for a flyby of Kuiper Belt object 2014 MU69 on January 1, 2019, and Juno, an orbiting mission that is studying the origin, evolution, and internal structure of Jupiter. The spacecraft departed for near-Earth asteroid (101955) Bennu aboard an United Launch Alliance Atlas V 411 evolved expendable launch vehicle at 7:05 p.m. EDT on September 8, 2016, on a seven-year journey to return samples from Bennu. The spacecraft is on an outbound-cruise trajectory that will result in a rendezvous with Bennu in November 2018. The science instruments on the spacecraft will survey Bennu to measure its physical, geological, and chemical properties, and the team will use these data to select a site on the surface to collect at least 60 g of asteroid regolith. The team will also analyze the remote-sensing data to perform a detailed study of the sample site for context, assess Bennu’s resource potential, refine estimates of its impact probability with Earth, and provide ground-truth data for the extensive astronomical data set collected on this asteroid. The spacecraft will leave Bennu in 2021 and return the sample to the Utah Test and Training Range (UTTR) on September 24, 2023.

     

基于最小二乘法的磁力计误差补偿与校准

磁力计在行人自主导航系统中用于提供绝对航行信息,而航向的精度直接决定着系统定位的精度。针对目前磁力计标定方法中存在磁干扰等问题,提出了一种基于最小二乘法和"8"字校准法对磁力计零偏进行实时校准的方法。该方法先利用最小二乘法修正磁力计零偏,再根据磁力计的模值大小及方差作为磁干扰的判断条件,用"8"字旋转方式进行实时校准。通过仿真和实验验证,新的方法有效地解决了磁力计误差补偿问题,证明了改进误差补偿算法的可行性和有效性。     

Experimental research on rotating detonation with liquid hypergolic propellants

This paper describes experimental research into the initiation and propagation of rotating detonation for liquid Nitrogen TetrOxide (NTO) and liquid MonoMethylHydrazine (MMH). An annular rocket-type combustor without nozzle was designed to investigate detonation combustion. The propellants were injected through unlike impingement injectors. The combustion flame fronts and pressure waves were detected using optical diagnostics and dynamic pressure sensors, respectively. The propagation of rotating detonation was established spontaneously by increasing the mass flow rate of propellants. The velocity of propagation of the flame fronts and pressure waves was nearly equal and reaches supersonic speed. Two different detonation combustion patterns are present, single wave mode and double waves mode. And in double waves mode, the two detonation waves are always counter-rotating. The possibility of rotating detonation initiation in a combustor with nozzle was also checked. Stable rotating detonation can be initialized and sustained at similar operating conditions.     

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.     

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。     

空间翻滚非合作目标消旋技术发展综述

大量残存太空的空间垃圾对在轨运行航天器的安全构成严重威胁,对其进行主动移除已迫在眉睫。火箭末级、失效卫星等非合作目标已失去姿态调整能力,且长期在失控状态下运行,受太阳光压、重力梯度等摄动力矩及失效前自身残余角动量等因素的影响往往会出现翻滚运动。对翻滚非合作目标直接捕获存在碰撞风险,为降低风险系数采取消旋后再捕获是较为合适的方式。在对火箭末级、失效卫星等典型非合作目标运动形式及消旋过程进行分析的基础上,综述了目前国内外所提出的接触式及非接触式消旋方法,并对非合作目标翻滚运动测量及动力学参数辨识和消旋控制这两项消旋共性关键技术进行了归纳总结。本综述将为中国空间碎片主动清除技术的发展提供有益参考。     

航空发动机两级反向旋流燃烧室燃烧流场大涡模拟研究

为深入了解真实航空发动机内燃烧流场,采用动态亚网格模型结合单步快速化学反应(FC)、火焰面(FLM)及反应进度变量(FPV)等三种燃烧模型对径向两级反向旋流燃烧室单头部构型进行了大涡模拟。为避免模型简化误差,对燃烧室包括全部气膜冷却孔在内的精细结构进行了完全仿真。在已达到统计定常状态的冷态流场基础上首先模拟了燃料喷注和掺混过程,约2.6ms后燃料到达真实的点火位置,随后采用FPV模型在半径3mm的球形区域数值模拟了点火,展示了在主燃孔横向射流作用下初始火焰沿化学恰当比混合分数等值线传播并充满整个火焰筒的发展过程,结果显示火焰到达燃烧室出口的耗时约为6～7ms。不同模型算法预测的平均温度场与CARS测量结果作了对比,LES-FPV,RANS-FPV,LES-FLM以及参考文献中RANS-FLM计算平均误差分别为3.47%,4.17%,7.76%和11.22%,表明LES改进了模拟精度,且FPV模型显著优于FLM模型。RANS-FPV预测的出口存在严重热斑,导致其给出的出口温度分布因子(OTDF)及最大径向温度分布因子(RTDF)值分别达到0.593和0.313;LES-FPV结果均匀性最好,其预测值分别为0.284和0.193。