行星际空间MHD模拟激波跃变关系分析

分析了模拟得到的可以传播到1AU以远的日地空间磁流体力学激波与Rankine-Hugnoniot跃变关系的符合程度．通过对模拟激波的结构及其在传播过程中的演化进行的分析，提出了模拟激波的定位方法；基于所提出的定位方法，利用向长青提出的确定MHD激波局地参数的方法计算了模拟得到的激波与Rankine-Hugnoniot跃变关系的偏差．结果表明在激波传播到100Rs以后，激波对中前向快激波与Rankine-Hugnoniot关系的符合达到很高的程度，相对误差在10^-2数量级以内；并且在激波传播到150 Rs以后，相对误差在10^-3数量级以内．这个结果说明文中所使用的有限差分数值格式能较好地模拟激波．     

Acceleration of interplanetary pick-up ions and anomalous cosmic rays

It may not be doubted anymore that anomalous cosmic rays (ACRs) are produced in the heliosphere from interplanetary pick-up ions through their acceleration at the solar wind termination shock. However, there is no general agreement in the community of heliospheric researchers concerning the mechanism of injection of the pick-up ions into the shock acceleration. We discuss here three possible ways for pick-up ions to be involved into the acceleration process at the termination shock: (1) preacceleration of pick-up ions in the whole region from the Sun up to the termination shock by solar wind turbulences and interplanetary shock waves, (2) local preacceleration of pick-up ions in a vicinity of the termination shock by shock surfing, and (3) formation of high-velocity tails in pick-up ion spectra consisting of secondary pick-up ions which are produced in the supersonic solar wind due to ionization of energetic neutral atoms entering from the inner heliosheath.     

Using gamma-ray burst prompt emission to probe relativistic shock acceleration

It is widely accepted that the prompt transient signal in the 10 keV–10 GeV band from gamma-ray bursts (GRBs) arises from multiple shocks internal to the ultra-relativistic expansion. The detailed understanding of the dissipation and accompanying acceleration at these shocks is a currently topical subject. This paper explores the relationship between GRB prompt emission spectra and the electron (or ion) acceleration properties at the relativistic shocks that pertain to GRB models. The focus is on the array of possible high-energy power-law indices in accelerated populations, highlighting how spectra above 1 MeV can probe the field obliquity in GRB internal shocks, and the character of hydromagnetic turbulence in their environs. It is emphasized that diffusive shock acceleration theory generates no canonical spectrum at relativistic MHD discontinuities. This diversity is commensurate with the significant range of spectral indices discerned in prompt burst emission. Such system diagnostics are now being enhanced by the broad-band spectral coverage of bursts by the Fermi Gamma-Ray Space Telescope; while the Gamma-Ray Burst Monitor (GBM) provides key diagnostics on the lower energy portions of the particle population, the focus here is on constraints in the non-thermal, power-law regime of the particle distribution that are provided by the Large Area Telescope (LAT).     

一种气动式冲击响应谱试验系统的设计与分析

大多数航天器单机产品都要求进行冲击响应谱试验,试验量级普遍为1000g~2000g,甚至超过3000g。对于较大质量(如50 kg以上)产品高量级的冲击试验,振动台、传统的摆锤式或跌落式冲击试验台均很难满足相关要求。文章研究并设计了一套能够进行大质量受试产品高量级冲击响应谱试验的气动冲击试验系统。该系统利用压缩空气瞬间释放膨胀推动质量块加速撞击具有多阶固有频率的谐振板,通过谐振板被激起的响应模拟复杂的衰减正弦波。测试结果表明,系统空载时冲击谱量级达8000g,负载200 kg时可达5000g,时域曲线为振荡衰减波,持续时间小于10 ms。文章提出的气动式冲击响应谱试验系统设计方法可为此类冲击试验系统的设计提供参考和理论依据。     

一种修正的Osher通量在高阶WCNS中的特性

将一种基于多维修正的Osher通量运用于高阶加权紧致非线性格式(WCNS)中,该修正通量主要在垂直于激波面的界面上增加耗散,能够改善Osher通量的激波捕捉稳定性,同时对边界层和接触间断的分辨率影响非常小。对修正的Osher通量在高阶WCNS中的特性进行研究,通过数值模拟测试了基于Osher通量的WCNS的激波稳定性、热流预测精度、边界层模拟能力、激波边界层干扰模拟能力,并与Steger-Warming通量和Roe通量进行了对比。结果表明修正后的Osher通量比Harten修正的Roe通量具有更好的激波捕捉鲁棒性,而边界层、驻点热流值和激波边界层干扰的模拟则明显优于Steger-Warming通量。上述结果说明了基于修正的Osher通量的高阶WCNS具有较好的激波捕捉特性、热流预测精度和边界层计算能力。     

Prediction of shock-layer ultraviolet radiation for hypersonic vehicles in near space

A systemic and validated model was developed to predict ultraviolet spectra features from the shock layer of near-space hypersonic vehicles in the ‘‘solar blind" band region. Computational procedures were performed with 7-species thermal non-equilibrium fluid mechanics, finite rate chemistry, and radiation calculations. The thermal non-equilibrium flow field was calculated with a two-temperature model by the finite volume technique and verified against the bow-shock ultra-violet(BSUV) flight experiments. The absorption coefficient of the mixture gases was evaluated with a line-by-line method and validated through laboratory shock tube measurements. Using the line of sight(LOS) method, radiation was calculated from three BSUV flights at altitudes of 38,53.5 and 71 km. The investigation focused on the level and structure of ultraviolet spectra radiated from a NO band system in wavelengths of 200–400 nm. Results predicted by the current model show qualitative spatial agreement with the measured data. At a velocity of 3.5 km/s(about Mach11), the peak absolute intensity at an altitude of 38 km is two orders of magnitude higher than that at 53.5 km. Under the same flight conditions, the spectra structures have quite a similar distribution at different viewing angles. The present computational model performs well in the prediction of the ultraviolet spectra emitted from the shock layer and will contribute to the investigation and analysis of radiative features of hypersonic vehicles in near space.     

LENS风洞试验返回器模型气动热特性模拟

国家数值风洞高超声速流动模拟软件HyFLOW的研制对打破国外同类软件的技术壁垒具有重要意义。与国外DPLR软件进行了对比研究，同时系统介绍了HyFLOW软件求解器的数值方法、物理化学模型以及壁面催化特性计算模型等主要方法，采用典型算例对有限催化模型进行了数值验证，最后基于LENS风洞试验146 mm返回器标模外形开展了高超声速气动热特性数值模拟。研究结果表明，HyFLOW软件在高超声速热化学非平衡流动模拟与评估方面的气动力计算精度高，与国外同类软件DPLR相当，同时其壁面催化条件下的气动热计算精度可靠，可信度高。     

前后缘型线同时可控的乘波体设计

提出了一种前后缘型线同时可控的乘波体设计方法,在马赫数可控的外锥形曲面基准流场中,结合流线追踪技术和混合函数,实现了椭圆前缘转椭圆后缘的乘波体设计,并在设计点(Ma=6.0)和接力点(Ma=4.0)对其进行数值仿真研究。前后缘同时可控的乘波体在型面剧烈过渡处产生了较弱的激波,出口两侧存在高温高压区,后部对称面附近的激波形状由圆弧变为平直线且出口处流场基本均匀,非常有利于与进气道匹配设计。另外,该乘波体具有较高的容积率和预压缩效率,附面层修正后的容积率为0.24,设计点时乘波特性较好,接力点时前部完全乘波,具有较高的升阻比,有黏条件下设计点和接力点的升阻比分别为2.54和2.41。此外,与给定前缘的乘波体相比,其升力、阻力、俯仰力矩和出口增压比都有明显增加,但是升阻比和出口总压恢复系数有所降低,在设计点无黏升阻比由3.56降为3.00。以上研究表明,本文的设计方法可行且更加灵活,拓宽了乘波体的选择范围。     

CARDC 激波风洞 TSP 技术研究进展

从基本原理、关键技术和验证应用三个方面总结了近两年在中国空气动力研究与发展中心激波风洞中开展的温敏涂层(TSP)技术相关研究工作。通过解决快速响应温敏发光材料研制、模型研制、数据处理等一系列关键技术,完成图像采集系统、光学系统及标定系统的配套和系统集成,建立了一套适于激波风洞试验的高速 TSP 测量及标定系统。该技术可在激波风洞试验中获取模型被测面温敏涂层的发光图像,基于该图像可以直接观察模型表面热流分布和捕捉峰值热流的准确位置。结合温敏发光材料的物性参数标定数据,能够实现对模型表面热流的定量测量。不同于传统的传感器点热流测量技术只能得到模型表面有限数量的离散点的热流值,TSP 技术能够以高空间分辨率得到较大面积区域的详细热流分布信息,可更加全面的测量模型外表面的热环境,并且可以据此进一步分析和辨别边界层流态以及确定边界层转捩位置。试验对比表明,TSP 技术的测量结果与点热流传感器的测量结果具有良好的一致性。目前该技术已趋于成熟,在Φ2 m 和Φ0.6 m 激波风洞上成功应用于边界层转捩研究、局部干扰区热环境研究和复杂外形飞行器热环境研究等领域,已成为激波风洞除点测热技术之外又一重要测热技术。     

后掠翼三维鼓包串激波控制参数的影响

针对跨声速后掠翼,三维鼓包串作为一种有效的减阻方式具有结构简单、高效及鲁棒性好等优点.利用全局优化算法探索了鼓包设计参数空间的整体特性,并对鼓包长度、三维鼓包展向设计参数对鼓包减阻效果的影响进行了研究,发现鼓包顶点位置和高度对阻力系数最敏感,三维鼓包的展向设计参数则对阻力系数不敏感,而鼓包长度和鼓包相对展长越长越有利于减阻.在此基础上开展了小后掠角自然层流机翼加3种不同类型鼓包串的优化研究,通过优化结果发现,增加优化后的三维鼓包串,可将小后掠角自然层流机翼阻力发散马赫数向后推移,并且鼓包平均长度和控制区越大,效果越好.三维鼓包串具有良好的局部控制特性,可用于局部较强激波的抑制.三维鼓包串对常规后掠翼波阻具有良好的控制效果,同时能够抑制激波诱导的机翼后缘气流分离.