双级涡流器环形燃烧室整体流场数值模拟

在任意曲线坐标系下对包括扩压器、双级涡流器及火焰筒在内的环形燃烧室三维两相燃烧整体流场进行数值模拟。由于环形燃烧室形状复杂,采用偏微分方程法与整体分区结合法生成环形燃烧室整体网格。所用的数学模型有:k-ε紊流模型、EBU-Arrhenius紊流燃烧模型、六通量热辐射模型以及颗粒群轨道模型等。在非交错网格系下,气相采用SIMPLE算法求解,液相采用PSIC算法求解。数值分析不同燃烧室进口气流参数以及涡流器几何尺寸对燃烧室流场的影响,并将计算结果与实验数据进行了比较。结果表明本文的计算方法合理性可用于环形燃烧室的研制与优化设计。     

Cr12MoV钢电火花辅助铣削实验研究

以典型难切削金属材料Cr12MoV模具钢为研究对象,使用ABAQUS对其在电火花放电条件下温度场进行数值模拟,在不同进给率下对其进行传统铣削和电火花辅助铣削对比试验。借助高速摄像机、扫描电镜和测力计等设备,对其切削力特征、表面形貌和刀具磨损进行了对比分析研究。结果表明,电火花辅助铣削的切削力比传统铣削降低28.57%～51.47%,表面粗糙度降低2/3。与传统铣削相比,电火花辅助铣削在降低切削力、提高表面质量和减少刀具磨损方面具有显著优势。     

概率有限状态机在动态效能评估中的应用

为了反映作战过程中实时战场变化对武器作战效能的影响，本文对武器作战动态效能评估(DEE)方法进行研究，提出一种基于概率有限状态机(PFSM)的动态效能评估方法。利用该方法对武器作战过程进行动态效能评估的同时，能够快速准确地分析影响武器作战效能的关键因素，为作战方案决策及武器研发提供依据。该方法考虑了武器装备、战场环境、作战方案及作战目标这四个战场信息空间对武器效能的影响，能够根据实时战场信息输出动态效能变化曲线。本文以反舰导弹为例，对其进行动态效能评估，结果表明,本文所提出的方法能够动态评估不同战场信息对效能的影响，并快速找到影响其效能的关键因素，从而为作战方案优化提供参考。     

火星进入舱开伞弹伞载荷动力放大系数研究与试验验证

Firstly, the analytical formulas of the dynamic magnification factor with the pulse time of the response spectrum of a single degree of freedom system under the rectangular and half sine pulse are derived. Then the parachute inflation and ejection low frequency high shock load dynamic simulation model of the Mars entry vehicle is built based on abaqus explict dynamics, and the influence of the shock load shape, load time and load damping are analyzed. Finally, the experiments of the opening parachute load suspension impact dynamic load and the parachute load real parachute impact dynamic load are carried out.The results show that the structure responds decline when the shock load time is less than  1 ms , and the static equivalence load becomes steady when the load time is longer than 5 ms; the dynamics equivalence load of the parachute inflation is about 1 time than static because of the smooth time wave, but the parachute ejection’s is about 1~2 times than static due to the steep rectangle wave.      

Statistical analysis of geomagnetic field variations during solar eclipses

We investigate the geomagnetic field variations recorded by INTERMAGNET geomagnetic observatories, which are observed while the Moon’s umbra or penumbra passed over them during a solar eclipse event. Though it is generally considered that the geomagnetic field can be modulated during solar eclipses, the effect of the solar eclipse on the observed geomagnetic field has proved subtle to be detected. Instead of exploring the geomagnetic field as a case study, we analyze 207 geomagnetic manifestations acquired by 100 geomagnetic observatories during 39 solar eclipses occurring from 1991 to 2016. As a result of examining a pattern of the geomagnetic field variation on average, we confirm that the effect can be seen over an interval of 180?min centered at the time of maximum eclipse on a site of a geomagnetic observatory. That is, demonstrate an increase in the Y component of the geomagnetic field and decreases in the X component and the total strength of the geomagnetic field. We also find that the effect can be overwhelmed, depending more sensitively on the level of daily geomagnetic events than on the level of solar activity and/or the phase of solar cycle. We have demonstrated it by dividing the whole data set into subsets based on parameters of the geomagnetic field, solar activity, and solar eclipses. It is suggested, therefore, that an evidence of the solar eclipse effect can be revealed even at the solar maximum, as long as the day of the solar eclipse is magnetically quiet.     

Dual-frequency carrier smoothed code filtering with dynamical ionospheric delay modeling

In GNSS applications, carrier-smoothed-code is a widely used technique to combine code pseudo-range and carrier phase measurements. A dynamical ionospheric delay modeling method is proposed based on Kalman filter and least-squares theory. The level of the process noise is adaptively tuned along with the real-time KF state estimation, based on the online variance component estimation method. Meanwhile, the correlations of the time differenced carrier phase measurements are considered. This approach avoids overly optimistically evaluating the estimate and improves the transient accuracy of the estimates. A real GPS dataset is employed to check the performance of the proposed method under different conditions. The results show that the new algorithm can model the ionospheric delay variation well with different sampling intervals or even in ionospheric abnormal environment. The positioning accuracy can be confirmed, about 21%, 35% and 16% better are obtained in the N, E, and U direction than raw dataset.     

皮卫星星箭分离动力学模拟及其灵敏度分析

皮卫星能源有限、姿控能力差等特点决定其对星箭分离初始姿态要求较高。在采用自主研发的皮卫星星箭分离机构的基础上,以多体动力学理论为基础,采用ADAMS软件建立了皮卫星及其星箭分离机构虚拟样机模型,分别就皮卫星质心偏离量、分离弹簧与舱门扭簧弹性系数对入轨初始姿态影响展开了分析。分析结果表明：质心偏心量对分离姿态影响最明显,分离弹簧与舱门扭簧弹性系数对其影响次之,合理配置分离弹簧与舱门扭簧弹性系数有利于卫星保持良好的姿态分离。在轨分离试验显示：分离时刻皮卫星滚动角速度、俯仰角速度、偏航角速度分别为-0.18（°）/s,-1.6（°）/s,0.95（°）/s,与在轨环境下仿真结果基本相符;入轨初始姿态能满足皮卫星的姿控要求,为其后续工作提供了保障。     

基于粒子群优化核极限学习机的北斗超快速钟差预报

针对卫星钟差序列中非线性特性较为复杂和超快速钟差预报精度较低的问题,将核极限学习机算法引入到北斗超快速钟差预报中。首先,将极限学习机进行优化,引入粒子群优化算法来选择核极限学习机所需的核参数和正则化参数;然后,将优化后的方法应用到超快速钟差预报中,并给出了利用该方法进行超快速钟差预报的步骤;最后,在分析iGMAS提供的实测北斗超快速钟差数据的基础上,选用单天和多天数据进行短期预报。结果表明：在短期预报6h范围内,利用本文提供的优化方法解算得到的超快速钟差预报精度明显优于二次多项式模型和周期项模型,并且采用此方法得到的超快速钟差预报产品与iGMAS提供的超快速钟差预报产品(ISU-P)相比,GEO、IGSO和MEO卫星的预报精度分别提升了50.51%、46.98%、40.67%,其与最终精密钟差的符合程度显著 增强 。     

吸气式高超声速飞行器助推-巡航轨迹优化

针对吸气式高超声速巡航飞行器建立了纵向平面内的二维轨迹优化模型(包括火箭助推段和吸气式飞行段),其中大气模型、气动力模型和发动机模型均建立了比较详细的模型,能够比较全面、准确地描述吸气式高超声速巡航飞行器的特征;基于配点法建立了适用于高超声速巡航飞行器助推-巡航轨迹优化的方法,在求解非线性规划时引入了规范化处理、稀疏分析和偏导数计算方法等,以提高优化效率;对吸气式高超声速飞行器助推-巡航轨迹进行了优化研究,分析了典型设计参数变化对最优轨迹的影响。仿真结果表明:所建立的方法能够快速、高精度求解吸气式高超声速巡航飞行器轨迹优化问题,并且能够方便地分析设计参数变化对最优轨迹的影响,可用于吸气式高超声速飞行器飞行剖面设计与优化。     

试验箱风速对航天器部件常压低温热变形试验的影响分析

文章以航天器机械臂为研究对象,采用流-热-固耦合方法仿真分析了单一送风形式下,试验箱不同送风速度对机械臂常压低温热变形的影响,并进行了试验验证。分析发现:随着送风速度的增大,机械臂表面的温度场分布更均匀且温度值更接近于设定值,从而更有利于低温热变形试验的实施;但由于存在环境噪声,必须经过静置稳定后才可以进行变形测量。此分析结果可以用于指导航天器部件常压低温热变形试验更加精确、高效地实施。