低排放燃烧室化学反应器网络模型的参数化

为了掌握低排放燃烧室的污染物排放情况,对其化学反应网络器(CRN)模型的参数化进行研究.对爬升工况下燃烧室CFD数值模拟结果进行分析,划分燃烧室的结构,得到燃烧室的CRN模型.再利用自编程软件对燃烧室的结构参数和进口参数进行参数化定义,并把参数化的CRN模型在不同工况下的模拟结果与试验结果分别比较.结果表明:在慢车工况下二者相差不大,在爬升工况下二者差异也在允许误差范围之内.验证了该模型可行性较好,该参数化CRN模型可用于预测低排放燃烧室的污染物排放量和出口温度.     

油气比对燃气分析法燃烧效率、气态污染物测试精度的影响

在燃气分析单点测试偏差的基础上,针对燃气轮机、主燃烧室及加力燃烧室目前采用的取样方式的现状,建立了燃气分析法和流量法的油气比偏差对燃烧效率和气态污染物测试精度的影响规律。结果表明:对于采用移位机构进行测量的主燃烧室,流量法和燃气分析法油气比相差在5.1%以内时,说明有足够的测点密度,数据有效,此时的燃烧效率精度优于0.5%;对于加力燃烧室和整机测试,由于取样点不足,油气比偏差较大,燃烧效率的精度还取决于油气比和CO的体积分数。保证足够的取样点密度是燃气分析测试结果具有较高精度的前提。      

液体射流喷入横向气流混合特性研究进展简

 随着低污染燃烧技术的发展,液体射流在横向亚声气流中的液雾混合特性越来越受到关注。因此对液体射流在横向亚声气流中的研究进展进行了综述,综述内容主要包括3个方面：液体射流在横向气流中雾化破碎;液体射流的穿透深度;液雾在横向气流中的散布和输运。大部分研究工作是针对单个直射式液体射流喷入均匀横向气流中的,也有研究考察了燃油脉动、气流不均匀或者旋转气流条件下射流在横向气流中的混合特性,然而对多喷射点或气动雾化直射式喷嘴形成的液雾在横向气流中的混合特性的研究工作开展的相对较少。最后对液体射流在横向气流中的国内外试验研究工作进行了简要的概括。通过对国内外相关研究进展的概括,并且以先进航空发动机低排放燃烧室中的雾化方式为背景,提出了液体横向射流混合特性研究应进一步完善的工作内容。     

传导发射测量不确定度评定的验证

为了保证测量不确定度评定结果有足够的可信度,必须对评定的测量不确定度进行验证。概述了采用蒙特卡洛模拟法验证传导发射测量不确定度的方法,介绍了通过埃奇沃思级数估计测量结果概率分布的过程和应用蒙特卡洛方法解决实际问题的基本步骤,最后结合某试验室的实例给出了验证结果,证明在大部分频点上其根据GUM评定的传导发射测量不确定度是可信的。     

Equilibration Processes in the Warm-Hot Intergalactic Medium

The Warm-Hot Intergalactic Medium (WHIM) is thought to contribute about 40–50% to the baryonic budget at the present evolution stage of the universe. The observed large scale structure is likely to be due to gravitational growth of density fluctuations in the post-inflation era. The evolving cosmic web is governed by non-linear gravitational growth of the initially weak density fluctuations in the dark energy dominated cosmology. Non-linear structure formation, accretion and merging processes, star forming and AGN activity produce gas shocks in the WHIM. Shock waves are converting a fraction of the gravitation power to thermal and non-thermal emission of baryonic/leptonic matter. They provide the most likely way to power the luminous matter in the WHIM. The plasma shocks in the WHIM are expected to be collisionless. Collisionless shocks produce a highly non-equilibrium state with anisotropic temperatures and a large differences in ion and electron temperatures. We discuss the ion and electron heating by the collisionless shocks and then review the plasma processes responsible for the Coulomb equilibration and collisional ionisation equilibrium of oxygen ions in the WHIM. MHD-turbulence produced by the strong collisionless shocks could provide a sizeable non-thermal contribution to the observed Doppler parameter of the UV line spectra of the WHIM.     

Thermodynamical Properties of the ICM from Hydrodynamical Simulations

Modern hydrodynamical simulations offer nowadays a powerful means to trace the evolution of the X-ray properties of the intra-cluster medium (ICM) during the cosmological history of the hierarchical build up of galaxy clusters. In this paper we review the current status of these simulations and how their predictions fare in reproducing the most recent X-ray observations of clusters. After briefly discussing the shortcomings of the self-similar model, based on assuming that gravity only drives the evolution of the ICM, we discuss how the processes of gas cooling and non-gravitational heating are expected to bring model predictions into better agreement with observational data. We then present results from the hydrodynamical simulations, performed by different groups, and how they compare with observational data. As terms of comparison, we use X-ray scaling relations between mass, luminosity, temperature and pressure, as well as the profiles of temperature and entropy. The results of this comparison can be summarised as follows: (a) simulations, which include gas cooling, star formation and supernova feedback, are generally successful in reproducing the X-ray properties of the ICM outside the core regions; (b) simulations generally fail in reproducing the observed “cool core” structure, in that they have serious difficulties in regulating overcooling, thereby producing steep negative central temperature profiles. This discrepancy calls for the need of introducing other physical processes, such as energy feedback from active galactic nuclei, which should compensate the radiative losses of the gas with high density, low entropy and short cooling time, which is observed to reside in the innermost regions of galaxy clusters.     

Kuafu and the studies of CME initiation

We first briefly review the current trend in the studies of coronal mass ejections (CMEs), then summarize some recent efforts in understanding the CME initiation. Emphasis has been put on the studies of Earth-directed CMEs whose associated surface activity and large scale magnetic source have been well identified. The data analysis by combining the MDI full disc magnetograms, vector magnetograms of active regions, EUV waves and dimmings, non-thermal radio sources, and the SOHO LASCO observations has shed new light in understanding the CME magnetism. However, the current studies seem to invoke new observations in a few aspects: (1) The observations which enable us to trace CMEs from the earliest associated surface activity to its initial acceleration and key development in the low corona in the height of 1–3 R; (2) The imaging spectroscopic observations which can be used to diagnose the early plasma outflow and the line-of-sight velocity in understanding the kinematics of CMEs; (3) The accurate timing from primary magnetic energy release, manifested by chromospheric activity, non-thermal radio bursts, and EUV, X-ray and γ-ray emissions, to the CME initiation, early acceleration and propagation, and the consequences in the interplanetary space and magnetosphere. The Kuafu Mission will meet the basic requirement for the new observations in CME initiation studies and serve as a monitor of space weather of the Sun–Earth system.     

空间碎片撞击在轨感知技术研究综述

随着航天发射活动的日益频繁,空间碎片环境随之恶化。为了应对空间碎片的撞击威胁,人们提出了用空间碎片撞击在轨感知系统实时监测航天器在轨遭受空间碎片撞击的情况。文章在对国内外相关研究机构研究成果的调研基础上,介绍了国内外在空间碎片撞击在轨感知技术领域的研究现状,对各国基于超高速撞击声发射技术的空间碎片撞击在轨感知技术的发展状况进行了全面评述,重点介绍了国内的研究进展。最后基于国内航天事业需要,探讨了未来发展方向。     

碳纤维复合材料贮箱内压和低温承载行为研究

碳纤维增强聚合物复合材料具有轻质高强的优异特性,是液氢液氧燃料贮箱的理想材料。然而液氢液氧燃料贮箱在服役时要承受极低温度载荷,复合材料贮箱箱体的低温结构可靠性尚未可知。开展了碳纤维/环氧复合材料缠绕贮箱结构在温度和内压载荷下的变形及损伤研究,分别进行了常温/低温抗渗漏测试,结合应变测量、声发射监测、氦质谱检漏等方法分别研究了内压以及低温工况对复合材料贮箱的应变分布及损伤泄漏状态影响机制。研究结果表明,封头与圆筒区域交界处易产生应变集中,低温载荷导致复合材料局部小幅度基体损伤及纤维/基体界面脱粘,但并未影响贮箱箱体承压性能和气密性。本研究可为未来大型航天器减质设计提供参考。     

Changes in the Structure of Comet Nuclei Due to Radioactive Heating

The initial structure of a comet nucleus is most probably a homogeneous, porous, fine-grained mixture of dust and ices, predominantly water. The water ice is presumably amorphous and includes considerable fractions of occluded gases. This structure undergoes significant changes during the early evolution of the nucleus at large heliocentric distances, due to internal radiogenic heating. Structural changes occur mainly as a result of gas flow through the porous medium: the gas pressure that builds up in the interior is capable of breaking the fragile structure and altering the pore sizes and porosity. These effects are modeled and followed numerically, testing a large number of parameters. This revised version was published online in June 2006 with corrections to the Cover Date.