Self-similar stochastic processes in solar wind turbulence

Solar wind data is used to estimate the autocorrelation function for the stochastic process x(τ) = y(t + τ) − y(t), considered as a function of τ, where y(t) is any one of the quantities B²(t), n_p(t)V²(t), or n_p(t). This process has stationary increments and a variance that increases like a power law τ^2γ where γ is the scaling exponent. For the kinetic energy density and the proton density the scaling exponent is close to the Kolmogorov value γ = 1/3, for the magnetic energy density it is slightly larger. In all three cases, it is shown that the autocorrelation function estimated from the data agrees with the theoretical autocorrelation function for a self-similar stochastic process with stationary increments and finite variance. This is far from proof, but it suggests that these stochastic processes may be self-similar for time scales in the small scale inertial range of the turbulence, that is, from approximately 10 to 10³ s.     

基于气化煤油喷注的RBCC燃烧室亚燃模态燃烧组织研究

针对RBCC发动机亚燃模态进行主动冷却的情况下,煤油发生气化后喷入燃烧室的燃烧组织开展研究。在亚燃模态低来流总温条件下,使用小流量富燃一次火箭高温射流作为引导火焰可以实现支板喷注二次燃料的可靠点火和稳定燃烧,当煤油喷注前加热到气化/超临界态时,燃烧室最高压力相比于室温液态煤油提高约10%左右。当关闭一次火箭后,利用凹腔成功实现火焰稳定,而使用室温液态煤油喷注时,凹腔内无法实现火焰稳定。通过数值模拟获得了不同喷注方案的燃烧室燃烧流场特征和燃烧组织过程,为进一步优化燃烧室的性能提供依据。结果分析表明通过合理布置燃料支板喷注位置,由燃料支板下游集中的燃料热释放使得气流在扩张燃烧室构型中实现"热力壅塞",通过燃料分配实现燃烧室内合理的燃烧释热分布,使RBCC发动机亚燃模态完成高效燃烧组织。     

Coupled Lagrangian impingement spray model for doublet impinging injectors under liquid rocket engine operating conditions

To predict the effect of the liquid rocket engine combustion chamber conditions on the impingement spray, the conventional uncoupled spray model for impinging injectors is extended by considering the coupling of the jet impingement process and the ambient gas field. The new coupled model consists of the plain-orifice sub-model, the jet-jet impingement sub-model and the droplet collision sub-model. The parameters of the child droplet are determined with the jet-jet impingement sub-model using correlations about the liquid jet parameters and the chamber conditions.The overall model is benchmarked under various impingement angles, jet momentum and offcenter ratios. Agreement with the published experimental data validates the ability of the model to predict the key spray characteristics, such as the mass flux and mixture ratio distributions in quiescent air. Besides, impinging sprays under changing ambient pressure and non-uniform gas flow are investigated to explore the effect of liquid rocket engine chamber conditions. First, a transient impingement spray during engine start-up phase is simulated with prescribed pressure profile. The minimum average droplet diameter is achieved when the orifices work in cavitation state, and is about 30% smaller than the steady single phase state. Second, the effect of non-uniform gas flow produces off-center impingement and the rotated spray fan by 38°. The proposed model suggests more reasonable impingement spray characteristics than the uncoupled one and can be used as the first step in the complex simulation of coupling impingement spray and combustion in liquid rocket engines.     

The role of radial perpendicular diffusion and latitude dependent acceleration along the solar wind termination shock

A numerical model, based on Parker’s transport equation, describing the modulation of anomalous cosmic rays and containing diffusive shock acceleration is applied. The role of radial perpendicular diffusion at the solar wind termination shock, and as the dominant diffusion coefficient in the outer heliosphere, is studied, in particular the role it plays in the effectiveness of the acceleration of anomalous protons and helium when its latitude dependence is changed. It is found that the latitudinal enhancement of radial perpendicular diffusion towards the heliospheric poles and along the termination shock has a prominent effect on the acceleration of these particles. It results in a ‘break’ in the energy spectrum for anomalous protons at ∼6.0 MeV, causing the spectral index to change from E^−1.38 to E^−2.23, but for anomalous helium at ∼3.0 MeV, changing the spectral index from E^−1.38 to E^−2.30. When approaching the simulated TS, the changes in the modulated spectra as they unfold to a ‘steady’ power law shape at energies below 50 MeV are much less prominent as a function of radial distances when radial perpendicular diffusion is increased with heliolatitude.     

网格计算在工业过程控制中的应用前景

网格计算是一种新兴的解决大规模复杂问题的应用技术,充分利用现有资源提供高性能的计算能力。现在的生产过程越来越向大规模复杂化方向发展,过程控制需要新的控制模型和控制方法来解决这些问题。但现有的计算能力无疑又限制了控制技术的应用,将高性能的网格计算运用到过程控制当中可以提高控制模型和控制算法的计算速度,也将大大提高其控制品质和应用范围。     

航天器发动机再启动的微重力基础研究

介绍了发动机再启动问题的工程应用背景，阐述了涉及发动机再启动的微重力基础研究，范畴。在微重力条件下，正确考虑外界干扰载荷对贮箱中流体动力学行为的影响是至关重要的。给出了用三维程序计算的一些结果。     

超临界环境下煤油替代物液滴燃烧特性数值研究

为研究液氧/煤油火箭发动机燃烧室内经喷注形成的煤油液滴的燃烧过程，基于实际气体状态方程、高压热物性修正、高压气液平衡和详细化学反应动力学，建立一维的全瞬态液滴燃烧模型，对超临界环境下两组分煤油替代物液滴的燃烧特性及液滴初始直径的影响进行仿真研究。结果表明，在超临界环境下，相比于煤油液滴纯蒸发过程，煤油液滴燃烧过程的迁移时刻大大提前；煤油液滴着火之后很快进入超临界燃烧阶段，此时液滴燃烧过程可以看成中心附近的燃料高浓度区与外侧氧气高浓度区之间的扩散燃烧过程；煤油液滴的火焰半径先增大，达到最大值之后开始减小，并减小为零，火焰温度在着火之后快速上升至最大值，并基本保持不变，在火焰半径减小为零之后开始降低；随着液滴初始直径的增大，火焰特性以及液滴中心参数变化曲线趋势不变、整体延迟，着火时间、迁移时间和液滴寿命增大。     

空间站燃烧科学实验系统设计

建立空间站燃烧实验系统，可满足未来空间微重力燃烧实验系统需求.通过空间站微重力燃烧实验研究，可拓展空间燃烧学研究.根据所要实现的功能及燃烧实验需求，对中国空间站燃烧柜的燃烧科学实验系统进行了设计和分析.燃烧科学实验系统由8个子系统组成，是一个适合开展气、液、固多种燃料燃烧实验的综合性实验系统.考虑到强度设计要求，在完成方案设计后，对系统进行了有限元分析，并在研制的结构件上进行了力学环境实验.实验与分析结果表明，本文设计的实验系统能够满足环模实验的要求，结构合理可行.      

硼笼化合物对含铝液固高能燃料点火及燃烧性能的影响

为了探究硼笼化合物对液固凝胶型高能燃料的点火及燃烧性能的影响,采用高密度碳氢燃料MCRI-1、辅助分散剂胶凝剂和纳米铝粉为原料,制备了系列含铝液固凝胶型高能燃料(简称含铝高能燃料),并考察了含铝高能燃料的组成对其分散稳定性(即凝胶成型效果)的影响。在此基础上,考察了三种硼笼化合物对含铝高能燃料的密度、热值、点火及燃烧性能的影响。结果表明,提高胶凝剂含量或固液质量比(Al/MCRI-1)均可提高含铝高能燃料的分散稳定性。含铝高能燃料的密度和体积热值随着硼笼化合物的添加略有降低,但其质量热值在添加硼笼T和硼笼A后分别增加了11.6%和12.4%。硼笼化合物可将含铝高能燃料的燃温峰值提高21.1%～52.9%,点火延迟缩短44.5%～65.2%。硼笼化合物明显改善了含铝高能燃料的点火及燃烧性能。整体上,硼笼A添加效果最佳,且热解及燃烧可产生较多的气体,一定程度上增强了含铝高能燃料的膨胀做工能力。     

液体发动机燃烧室流场模拟的并行SIMPLE算法

用串行和并行ＳＩＭＰＬＥ算法对液体火箭发动机燃烧室内的复杂流动进行了数值模拟。控制方程组用欧拉坐标系下的Ｎ－Ｓ方程组描述。在并行虚拟机环境下研究了交错网格系统中参数的传输和接受模式, 从计算结果可以看出并行计算的效率较高, 是解决此类复杂流动大规模数值模拟问题的有效手段之一。