改进联邦滤波器在小卫星姿态确定中的应用

采用微小卫星姿态运动学、动力学方程,以磁强计／太阳敏感器为姿态敏感器进行姿态确定,研究了一种基于融合反馈的改进联邦滤波算法,提出了一种基于观测新息修改的信息分配原则。给出了由四元数描述卫星姿态的误差状态方程,并对观测矢量进行推导,获得了基于角速度的观测方程,丰富了观测模型。仿真结果表明：基于角速度观测方程的引入,增强了观测信息的利用率,进而提高了姿态确定的精度,降低了计算量,保证了可靠性。     

耦合凝相-气相动力学机理的二硝酰胺铵燃烧模型

为了研究二硝酰胺铵ADN(Ammonium Dinitramide)固体推进剂燃烧物理化学过程并预测其燃 烧特性,建立一个耦合凝相-气相动力学机理的ADN燃烧模型。该模型基于凝相与气相的总连 续方程、组元连续方程、能量守恒方程及有限速率化学动力学方程而建立,并引入多组元系 统状态方程封闭方程组。模型中包含34种组元,1个固相（凝相）ADN分解总化学反应和165 个气相细节（基元）化学反应,并使用以温度函数表示的物性参数进行计算。应用气相燃烧 模型 对0.6 MPa下ADN燃烧火焰温度、组元摩尔浓度分布进行预测;应用耦合凝相-气相的燃烧模 型对0.2 MPa～36 MPa压强区域内柱状端燃ADN推进剂燃速、燃烧表面温度进行预测,计算结 果与文献报道试验数据较吻合。说明该燃烧模型能够较准确描述ADN气相燃烧波结构和ADN固 体推进剂燃速特性。
     

八自由度弹架系统建模研究

本文结合某型号火箭箱式发射系统设计，建立了八自由度多联装火箭系统的模型，并对模的新方法及特点进行了分析研究 。     

压缩空气瓶内凝结水水位检测方法的探讨

由于压缩空气瓶在使用过程中会出现瓶内残留凝结水的现象,从而影响压缩空气瓶的容积,并产生化学腐蚀,影响气瓶的整体强度和耐压性能及其的寿命。为此,应掌握气瓶内凝结水水位情况,并且提高检测水位准确度。提出了一种利用气体状态方程来计算压缩空气瓶的冷凝水水位新见解,对压缩空气瓶的安全使用具有重要意义。     

物—伞系统运动稳定性初探

弹道－升力式再入飞行器常采用旋成体外形，但其质心偏离对称轴（纵轴）设置。这种飞行器在着陆前要采用降落伞作为主减速手段。研究质心偏离对称轴的旋成体与降落伞组成的系统的运动稳定性是一项有工程实践意义的课题。作为一种初步探索，在把降落伞视作刚体的条件下，按该系统平面运动方程考察其在平衡状态附近的稳定性，给出了运动稳定性判据。     

Understanding high-density matter through analysis of surface spectral lines and burst oscillations from accreting neutron stars

We discuss millisecond period brightness oscillations and surface atomic spectral lines observed during type I X-ray bursts from a neutron star in a low mass X-ray binary system. We show that modeling of these phenomena can constrain models of the dense cold matter at the cores of neutron stars. We demonstrate that, even for a broad and asymmetric spectral line, the stellar radius-to-mass ratio can be inferred to better than 5%. We also fit our theoretical models to the burst oscillation data of the low mass X-ray binary XTE J1814-338, and find that the 90% confidence lower limit of the neutron star’s dimensionless radius-to-mass ratio is 4.2.     

Kinetics of gas-Grain Reactions in the Solar Nebula

Thermochemical equilibrium calculations predict gas phase, gas-grain, and solid phase reactions as a function of pressure and temperature in the solar nebula. However, chemical reactions proceed at different rates, which generally decrease exponentially with decreasing temperature. At sufficiently low temperatures (which vary depending on the specific reaction) there may not have been enough time for the predicted equilibrium chemistry to have taken place before the local environment cooled significantly or before the gaseous solar nebula was dispersed. As a consequence, some of the high temperature chemistry established in sufficiently hot regions of the solar nebula may be quenched or frozen in without the production of predicted low temperature phases. Experimental studies and theoretical models of three exemplary low temperature reactions, the formation of troilite (FeS), magnetite (Fe₃O₄), and hydrous silicates, have been done to quantify these ideas. A comparison of the chemical reaction rates with the estimated nebular lifetime of 0.1-10 million years indicates that troilite formation proceeded to completion in the solar nebula. Magnetite formation was much slower and only thin magnetite rims could have formed on metal grains. Hydrous silicate formation is predicted to be even slower, and hydrous silicates in meteorites and interplanetary dust particles probably formed later on the parent bodies of these objects, instead of in the solar nebula. This revised version was published online in June 2006 with corrections to the Cover Date.     

PAC,PAM复合絮凝剂处理不同浊度水的动力学和机理研究

本文系统了无机高分子铝盐ＰＡＣ与有机高分子ＰＡＭ复合絮凝剂处理不同浊度水的絮凝效果、性能和机理。测定了最佳投药量、最佳水力条件及余浊变化、密度变化等，并一微摄影后摄了絮凝过程不同阶段的矾花大小。为管式絮凝器用于处理不同浊度术的设计研制提供了理论依据。 处     

物体—双伞系统运动方程与稳定性判据

利用刚体－双刚体模型给出了物体－双伞系统的运动方程与一种简化模式，并按运动稳定性分析的原理求得了该系统的稳定性判据。     

火箭煤油热裂解研究

为了探究火箭煤油热裂解过程以及抗氧化剂对热裂解过程的影响,通过火箭煤油静态热裂解实验研究了火箭煤油在683K～713K条件下裂解转化率、裂解产气率、气相产物组成随温度和时间的变化规律。同时,对比了加入1wt%抗氧化剂邻甲基对苯二酚(THQ)的火箭煤油热裂解行为,发现THQ对火箭煤油热裂解有明显抑制作用。683K～713K下,火箭煤油添加1wt%THQ前后的裂解活化能分别为150.0kJ/mol和210.5kJ/mol,并获得了相应的Arrhenius热裂解方程。对比发现我国火箭煤油裂解速率常数小于美国RP-1,RP-2火箭煤油。