一种星载扫描天线的分析与设计

为适应卫星平台的需要,达到卫星天线能够实现角度扫描(正负5度)和机械扫描结构尽可能简单的要求,本文设计了一种三反射镜配置结构的角度扫描天线。首先利用几何光学法设计了赋形面,然后确定了在不同的扫描角度时,平面镜移动到的位置点。最后,利用高斯衍射波束分析方法(Diffraction Guassian Beam Analysis)进行了电性能的仿真验证。结果显示,在所需角度的扫描范围内,其具有较高的主面孔径利用效率和扫描机械结构简单的特点。在兼顾角度扫描和机械扫描结构简单的条件下,天线达到了所需的性能要求。     

关于企业员工培训模式的研究

通过分析现阶段我国企业员工培训行为及新时代对员工培训的新要求，研究探讨了员工培训模式的基本架构及其关键环节。     

化学镀Ni-P合金涂层及其耐磨性

 对化学镀 Ni- P的硬度和耐磨性的关系进行了研究。低温长时加热可以获得高硬度 ,继续保温后其值不变。高温加热硬度达最大硬度以后保温硬度降低。不同温度处理其最大值相同 ,但耐磨性不同 ,高温处理优于低温处理。光电子能谱分析表明镀层表面富磷     

MESSENGER and the Chemistry of Mercury’s Surface

The instrument suite on the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) spacecraft is well suited to address several of Mercury’s outstanding geochemical problems. A combination of data from the Gamma-Ray and Neutron Spectrometer (GRNS) and X-Ray Spectrometer (XRS) instruments will yield the surface abundances of both volatile (K) and refractory (Al, Ca, and Th) elements, which will test the three competing hypotheses for the origin of Mercury’s high bulk metal fraction: aerodynamic drag in the early solar nebula, preferential vaporization of silicates, or giant impact. These same elements, with the addition of Mg, Si, and Fe, will put significant constraints on geochemical processes that have formed the crust and produced any later volcanism. The Neutron Spectrometer sensor on the GRNS instrument will yield estimates of the amount of H in surface materials and may ascertain if the permanently shadowed polar craters have a significant excess of H due to water ice. A comparison of the FeO content of olivine and pyroxene determined by the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) instrument with the total Fe determined through both GRNS and XRS will permit an estimate of the amount of Fe present in other forms, including metal and sulfides.     

Interstellar hydrogen bonding

This paper reports the first extensive study of the existence and effects of interstellar hydrogen bonding. The reactions that occur on the surface of the interstellar dust grains are the dominant processes by which interstellar molecules are formed. Water molecules constitute about 70% of the interstellar ice. These water molecules serve as the platform for hydrogen bonding. High level quantum chemical simulations for the hydrogen bond interaction between 20 interstellar molecules (known and possible) and water are carried out using different ab-intio methods. It is evident that if the formation of these species is mainly governed by the ice phase reactions, there is a direct correlation between the binding energies of these complexes and the gas phase abundances of these interstellar molecules. Interstellar hydrogen bonding may cause lower gas abundance of the complex organic molecules (COMs) at the low temperature. From these results, ketenes whose less stable isomers that are more strongly bonded to the surface of the interstellar dust grains have been observed are proposed as suitable candidates for astronomical observations.     

含Cs盐的HTPB/AP/Al复合推进剂特性研究

采用高倍率的扫描电镜观察了Cs盐的微观形貌,利用最小自由能法计算了不同含量Cs盐的复合推进剂能量性能并进行了测试,对Cs盐、含Cs盐复合推进剂的安全性能(撞击感度和摩擦感度)进行了评价,并对不同含量Cs盐推进剂的燃烧性能和燃烧火焰结构等性能进行了研究。结果表明,Cs盐的颗粒粒径较大,表面凹凸不平很不规则;含Cs盐复合推进剂的能量随Cs盐质量分数的增加稍有减小,推进剂密度从1.766 g/cm3提高到1.851 g/cm3;相对于AP,Cs盐和含Cs盐复合推进剂的感度均较低,当Cs盐含量为6%时,复合推进剂的机械感度最低,说明Cs盐在复合推进剂中应用是安全可行的;复合推进剂的燃速随Cs盐质量分数的增加而增大,当Cs盐含量为6%时,复合推进剂的压力指数降低幅度最大。     

On the physical state in the narrow-line region of the classical Seyfert galaxy NGC 7469

Based on the spectrophotometric data, by decomposition of the observed continuum, the power - law continuum characteristics of the central source are obtained. The behaviour of both electron temperature T_e and density n_e in the Narrow - Line Region (NLR) of NGC 7469 is discussed on the thermal and ionization equilibria calculations. T_e in NLR of the Sy1 galaxies are higher than the Sy2 ones, and the possible explanation is the lack of the dense (n_e 10¹⁰ cm⁻³) zone close to the central source in the Sy2 galaxies.     

船舶柴油机黑炭排放研究现状与展望

为进一步加强对船舶柴油机黑炭排放生成机理和特性的理解,探索有效的黑炭检测方法和排放控制技术,本文回顾有关船舶排放政策、黑炭定义、生成机理、理化特性、采样和测试以及控制技术等研究进展。指出加强包括火焰内颗粒形成与氧化机制以及润滑油的影响等船舶黑炭排放生成机理研究的必要性。论述船舶黑炭颗粒微观形貌、纳观结构、表面官能团、氧化活性、粒径尺寸、化学成分、元素组成等理化特性及影响。归纳黑炭排放测试与控制技术,建议结合多种检测方法,解决黑炭测试结果的不确定性问题。提倡借鉴车用柴油机成功经验,促进燃料、燃烧和尾气后处理技术的协同进步,实现船舶柴油机黑炭排放的有效控制。     

斜切径向旋流燃烧室主燃区光学测量与特性分析

针对斜切径向旋流环形燃烧室模型,采用可调谐二极管激光吸收光谱(TDLAS)、相干反斯托克斯喇曼光谱(CARS)光学测量手段,在模化状态(Case 2)下,对燃烧室主燃区进行温度测量,分别得到了主燃区内12个点的温度和沿两条路径的积分温度.使用Fluent 12.0对Case 2进行数值模拟,分别使用两种非预混燃烧模型:平衡化学反应模型(EM)和稳态层流小火焰(SLF)模型.通过将两种不同燃烧模型的计算结果与TDLAS,CARS试验测量数据作对比验证,发现EM计算得到的温度更高,并与试验测量温度更符合,其中与CARS测量的误差小于6%.在试验验证的基础上,完成燃烧室在冷流状态(Case 1)下的计算,分析主燃区的气流组织和主燃孔射流对回流区的影响;利用EM计算分析燃烧室主燃区在全压状态(Case 3)下燃料分布、温度场、组分分布和性能参数,如燃烧室的燃烧效率为0.97、出口温度分布系数为0.312等,较为全面反映了燃烧室内气流流动换热和燃烧现象.      

中尺度预报模式不同方案实验研究

以大雾天气为例,利用WRF中尺度数值预报模式对各物理参数进行调整,从而验证各物理方案对大雾形成和发展的作用,并将其与控制性实验进行比较。对水汽通量散度、雾区范围分析,结果表明：这三个敏感性实验都不能很好地反映实况,因此原控制性实验更适合做定量定性研究。