微重力场中对流—辐射—传质系统的地面模拟技术

研究了微重力条件下对流－辐射－传质稳态系统的地面相似模拟技术，进一步发 温度－材料综合保护技术。通过采取补偿热流，调整壁面热流密度分布的方法，保持了原型与尺寸适当缩小后的模型的Ｎｕ数，Ｓｈ数，材料，温度，湿度不变，从而实现模型与原型流动，换热和传质相似。     

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．     

防静电白色热控涂层的空间环境性能试验

通过在氧化锌晶格中掺入重金属离子，得到具有防静电功能的白色颜料，再以丙烯酸树脂为粘合剂制备出空间飞行器外表面用的ACR－1防静电白色热控涂层；研究了空间环境效应（包括紫外辐照，电子和质子辐照）对该热控涂层太阳吸收率的影响并与有机硅白色热控涂层进行了比较，地面模拟空间环境试验研究结果证明，ACR－1防静电白色热控涂层具有良好的空间稳定性。     

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).     

Numerical simulations of water spray on flame deflector during the four-engine rocket launching

This paper aims to study on the cooling effect with two types of water spray nozzle on the flame deflector during the four-engine launch vehicle take-off. To accurately simulate the two-phase flow of the rocket gas with multispecies and the water spray, the three-dimensional compressible Navier-Stokes equations, discrete ordinates methods and realizable k-Ɛ turbulence model are used to establish the rocket supersonic plumes impact model. The Eulerian dispersed phase (EDP) model was used to simulate the water spray into the exhaust gas. The accuracy and effectiveness of the gas-liquid flow model are verified by a good agreement between simulation results and experimental data. On this basis, a series of numerical simulation studies under different water injection position are performed. The results show that the high temperature regions, along the axis of engines on the deflector plate, have no significant temperature decreasing effect by water spray from the nozzles mounted on the apex of the deflector, and the high temperature converts a large quantity of water into vapor near the plume boundary, which would decrease the flow conductivity. With the cooling spray nozzle fixed directly to the deflector plate, the temperature decrease effect is obvious and the effect of thermal shock on deflector plate induced by exhaust plume is reduced, so that it can prevent the flame deflector from thermal ablation. The study results provide indepth information and engineering guidance for designing the water spray systems and increasing the safety of the launch process.     

A time-frequency analysis of the thermal radiation background anomalies caused by large earthquakes: A case study of the Wenchuan 8.0 earthquake

Strong earthquakes have an impact on the regional thermal radiation background, which has been both observed and confirmed. This effect produces anomalies in the thermal radiation background (TRBA) and increases the difficulty of extracting a thermal radiation anomaly (TRA) that is associated with an earthquake occurring during the same time period. The extraction and identification of such anomalies has been ignored by previous studies. In this study, we investigate the time-frequency analysis (TFA) method, together with the wavelet filtering of the Daubechies method and the relative power spectrum analysis of the Fourier Welch method to extract and analyse the TRBA caused by the 2008 Wenchuan Ms 8.0 earthquake and the TRA of the 2013 Minxian-Zhangxian Ms 6.6 earthquake using data concerning the brightness temperature of a black body (TBB) from the Fengyun-2 series of geostationary meteorological satellites developed by China. The result showed that this method can effectively extract and analyse the TRBA caused by the Wenchuan earthquake and the TRA of the Minxian-Zhangxian earthquake form a complex background environment. Furthermore, we discussed the impact of the earthquake on the TRBA and segmented the process. The impact is mainly reflected by three aspects; the characteristic period of the TRBA changes, the TRBA occurs at the same time every year, which is identical to the time at which the earthquake anomaly occurred, and the impact process is in stages. We also summarized the correlation between the characteristic parameters of a TRA and the regional thermal radiation background, geography, and climatic factors.     

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。     

基于自适应网格的超声速液体射流破碎过程研究

为研究超声速气流中液体横向射流的破碎过程,采用脉冲背景光方法和VOF方法开展了实验和数值研究。为提高液体横向射流中气液界面和气流场特征捕捉的精确性,采用自适应网格技术对于气液界面、激波出现位置进行网格细化,计算得到了较为精细的气液界面、激波特征及涡系结构。研究结果表明:在低成本仿真模拟条件下,利用自适应网格计算得到的射流轨迹和轮廓与实验吻合较好,射流轨迹的最大误差为10%;射流初始段在超声速气流条件下,仍然存在一段高度约为1.9倍喷孔直径且圆柱形态保持较好的连续光滑液柱。随着喷注压降的升高,液柱的长度逐渐增大;主流气体流经液柱发生三维绕流,在射流附近和近壁面区域形成不断演化的反转涡对,反转涡对的形成加速了液体射流一次破碎过程。