离心力场下多孔介质中热驱动换热的实验

以涡轮叶片新型超级冷却技术的研究为背景,在具有冷却通道的新型冷却结构中加入多孔介质,用实验的方法,模拟了离心力场下该新型冷却结构的热驱动换热现象,并与无多孔介质的情况进行了比较。实验结果表明:随着旋转速度、热流密度和冷气进口速度的增大,装有多孔介质的新型冷却结构的热驱动换热能力逐渐增强。同时实验研究发现,加入多孔介质后该新型冷却结构比未加多孔介质时具有更好的换热效果。      

民用高速旋翼飞行器发展战略分析及关键技术展望

面向直升机高速化的发展趋势,总结了国外高速旋翼飞行器的发展历程,开展了高速旋翼飞行器与直升机、通航飞机、公路、铁路等交通运输工具的效能仿真对比,基于潜在的民用市场需求,综合分析了高速旋翼飞机器在交通运输系统和应急救援体系中的优势与劣势。结果表明,民用高速旋翼飞行器在中国具有明确的战略发展定位,一方面可作为交通体系干支通、全网联的重要节点,以突出的任务效能融入交通运输应用体系;另一方面,面向中远程应急救援的需要,可满足敏捷救援体系响应速度的需求,填补现有直升机应用领域的空白。最后,针对重点发展构型,展望了中国未来民用高速旋翼飞行器的关键技术。     

旋转弹箭动态特性研究

针对防空反导用中口径舰炮制导炮弹动力学建模和动态特性,借鉴旋转导弹单通道控制的研究方法,在常规火箭弹外弹道模型的基础上建立有控弹道模型,对有控弹道模型进行线性化,并推导出短周期扰动运动弹体传递函数。仿真结果表明,在输入控制力的作用下,传递函数可应用于分析中口径舰炮制导炮弹在有控作用下的飞行稳定性与操纵性。     

Clusters of Galaxies: Setting the Stage

Clusters of galaxies are self-gravitating systems of mass ∼10¹⁴–10¹⁵ h ⁻¹ M_⊙ and size ∼1–3h ⁻¹ Mpc. Their mass budget consists of dark matter (∼80%, on average), hot diffuse intracluster plasma (≲20%) and a small fraction of stars, dust, and cold gas, mostly locked in galaxies. In most clusters, scaling relations between their properties, like mass, galaxy velocity dispersion, X-ray luminosity and temperature, testify that the cluster components are in approximate dynamical equilibrium within the cluster gravitational potential well. However, spatially inhomogeneous thermal and non-thermal emission of the intracluster medium (ICM), observed in some clusters in the X-ray and radio bands, and the kinematic and morphological segregation of galaxies are a signature of non-gravitational processes, ongoing cluster merging and interactions. Both the fraction of clusters with these features, and the correlation between the dynamical and morphological properties of irregular clusters and the surrounding large-scale structure increase with redshift. In the current bottom-up scenario for the formation of cosmic structure, where tiny fluctuations of the otherwise homogeneous primordial density field are amplified by gravity, clusters are the most massive nodes of the filamentary large-scale structure of the cosmic web and form by anisotropic and episodic accretion of mass, in agreement with most of the observational evidence. In this model of the universe dominated by cold dark matter, at the present time most baryons are expected to be in a diffuse component rather than in stars and galaxies; moreover, ∼50% of this diffuse component has temperature ∼0.01–1 keV and permeates the filamentary distribution of the dark matter. The temperature of this Warm-Hot Intergalactic Medium (WHIM) increases with the local density and its search in the outer regions of clusters and lower density regions has been the quest of much recent observational effort. Over the last thirty years, an impressive coherent picture of the formation and evolution of cosmic structures has emerged from the intense interplay between observations, theory and numerical experiments. Future efforts will continue to test whether this picture keeps being valid, needs corrections or suffers dramatic failures in its predictive power.     

模拟刷式封严泄漏流动的多孔介质模型

将刷束处理为多孔介质,在动量方程中引入由于多孔介质对流体流动的阻碍作用而引起的动量源项,之后详细分析了刷束孔隙率的确定方法并根据实验结果确定了该孔隙率,从而建立了模拟刷式封严泄漏流动的多孔介质模型.对该模型的计算结果做进一步的修正后,可以与实验结果很好地吻合,证明了利用该模型预测刷式封严的泄漏量是可行的.      

Composition of anomalous cosmic rays and implications for the heliosphere

We use energy spectra of anomalous cosmic rays (ACRs) measured with the Cosmic Ray instrument on the Voyager 1 and 2 spacecraft during the period 1994/157-313 to determine several parameters of interest to heliospheric studies. We estimate that the strength of the solar wind termination shock is 2.42 (–0.08, +0.04). We determine the composition of ACRs by estimating their differential energy spectra at the shock and find the following abundance ratios: H/He = 5.6 (–0.5, ⁺0.6), C/He = 0.00048 ± 0.00011, N/He = 0.011 ± 0.001, O/He = 0.075 ± 0.006, and Ne/He = 0.0050 ± 0.0004. We correlate our observations with those of pickup ions to deduce that the long-term ionization rate of neutral nitrogen at 1 AU is 8.3 × 10^–7 s^–1 and that the charge-exchange cross section for neutral N and solar wind protons is 1.0 × 10^–15 cm² at 1.1 keV. We estimate that the neutral C/He ratio in the outer heliosphere is 1.8(–0.7, +0.9) × 10^–5. We also find that heavy ions are preferentially injected into the acceleration process at the termination shock.     

飞机全,静压系统除水研究

阐述了全，静压系统中水的形成及其在导管中运动的方式，以及水柱移动的稳定位置与仪表的水柱误差指示值；提出了沉淀器的安装和管路的敷设要求。     

高温合金过滤中的界面问题研究

  过滤器吸附固态夹杂须满足两个条件:一是控制熔体的流动状态,使固态夹杂与过滤器相接触;二是熔体、过滤器及固态夹杂之间满足一定的界面能条件,使固态夹杂被过滤器吸附捕获,然后在高温下依靠热能将固态夹杂与过滤器烧结在一起。因此过滤器去除固态夹杂存在着三种机制;机械拦截机制、流体动力学机制及热力学机制。     

Deuterium Abundance in the Local ISM and Possible Spatial Variations

Excellent HST/GHRS spectra of interstellar hydrogen and deuterium Lyman- absorption toward nearby stars allow us to identify systematic errors that have plagued earlier work and to measure accurate values of the D/H ratio in local interstellar gas. Analysis of 12 sightlines through the Local Interstellar Cloud leads to a mean value of D/H = (1.50 ± 0.10) × 10-5 with all data points lying within ± 1 of the mean. Whether or not the D/H ratio has different values elsewhere in the Galaxy and beyond is a very important open question that will be one of the major objectives of the Far Ultraviolet Spectroscopic Explorer (FUSE) mission.     

压力传感器膜片表面温度的测量和分析计算

用红外热成象技术测量应变式压力传感器工作时的膜片温度分布,以判断由于电阻应变片工作时温度变化对测量准确性的影响。测量中为获得应变片的真实温度,作了表面喷黑处理。对于实用的3MPa和0.6MPa的压力传感器,在不同工作介质(空气和变压器油)及工作电压条件下进行了测量,其结果表明:应变片表面温度随工作电压增高而加大,且不均匀。以空气为介质的温度高于以变压器油为介质的温度。据此可以确定对压力测量准确度的影响。还用有限差分方法对压力传感器膜片表面温度作了数值分析计算。