Detached-eddy simulation of supersonic flow past a spike-tipped blunt nose

Space vehicle in atmosphere travels mostly at supersonic speed and generates a very strong bow shockwave around its blunt nose. Oblique shock and conical separated flow zone generated by a forward disk-tip spike significantly reduce the drag by reducing the high pressure area on the blunt nose. This study employs improved delayed detached eddy simulation to investigate the characteristic flow structures around a spike-tipped blunt nose at Mach number of 3 and Reynolds number(based on the blunt-body diameter) of 2.72x10~8. The calculated time-averaged quantities agree well with experimental data. Characteristic frequencies in different flow regions are extracted using fast Fourier transform. It is found that two distinct instability modes exist: oscillation mode and pulsation mode. The former is related to the foreshock/turbulence interaction with nondimensional frequency at around 0.004. The latter corresponds to the interaction between turbulence and shock structures around the blunt nose, with a typical coherent structure shedding frequency at 0.092.     

空间太阳能发电站拓扑架构及能量管理控制策略

针对超大功率空间太阳能电站(SSPS),提出了一种分布式+集中式系统拓扑架构,将系统电力传输分为太阳电池阵区、主结构电力传输区及发射天线阵区三大部分。根据系统三大阵区的能量流动关系,本文将SSPS系统的工作模式划分为最大功率点跟踪(MPPT)工作模式、跟踪功率指令工作模式及阴影区工作模式,并提出分层能源管理控制策略。最后,针对兆瓦级太阳电池阵的不同工作模式,利用Matlab/Simulink搭建空间太阳能电站系统仿真模型,进行仿真试验及对比分析,试验结果验证了拓扑架构的合理性及控制策略的有效性,为解决空间太阳能发电技术电力传输与能量管理问题提出了新思路。     

木星探测器轨道计算中的动力学

针对木星探测任务中轨道计算所面临的轨道动力学问题进行研究。首先，对木星探测轨道计算中涉及的时空参考系进行概述，比较了木星动力学时(TDJ)与质心动力学时(TDB)的差异；其次，对木星的定向参数模型及转换关系进行描述，给出了木星天球参考系与固联参考系的转换关系；再次，对木星探测器定轨计算中所需考虑的动力学模型进行讨论，提供了各类摄动加速度计算所需的公式；最后，对木星探测器JUNO的星历数据进行动力学拟合，检验了动力学模型的正确性。     

A star identification algorithm based on radial and dynamic cyclic features of star pattern

A full-sky star identification algorithm based on radial and dynamic cyclic patterns is presented with the aim of solving the “lost-in-space” problem. The dynamic cyclic pattern match is applied with a maximum cumulate comparison method to identify sensor-catalog pairings in initial match, which substantially eliminates the effects of the star position noise, magnitude noise, and false stars. After initial match pairings of stars are obtained, a chain part extension technique is employed to quickly search for the longest match chain as the final result. Experimental results indicate that the proposed algorithm is highly robust to star position noise, magnitude noise and false stars. In a series of simulations, the identification rate of the algorithm is 97.50% with 2.0 pixels star position noise, 96.90% with 0.4 Mv star magnitude noise and 95.30% with four false stars respectively. Moreover, the algorithm achieves an identification rate of 58.08% when only six stars are in the field of view.     

LL-SST的重力场测量类空间圆编队构型设计

根据LL-SST重力场测量改进对编队构型设计的要求,基于平均轨道根数描述的编队运动学方程,对自然轨道的编队构型进行了地球扁率二阶摄动下的修正,设计了在J2长期项和J3长周期项影响下相对稳定的类空间圆编队构型,并得到卫星的初始轨道根数.仿真表明,30天的仿真时间内,设计所得构型满足重力场测量下编队的约束,且在J2长期项和J3长周期项摄动影响下,与考虑J2半长轴修正设计的空间圆构型相比,在径向和迹向上的漂移量分别减少了99.980%,99.976%,法向振幅发散减少了99.710%.     

准静态电磁热弹性体第二类H-R型广义变分原理

应用变积方法建立了准静态电磁热弹性体的势能原理和第二类H-R型广义变分原理,并检验了变分原理的正确性,为电磁热弹多场问题的近似计算提供理论基础。     

热分析研究PET与某些高能氧化剂的相互作用

用高压差示扫描量热法(PDSC)和热重-微商热重法(TG-DTG),研究了PET与CL-20、DNTF、TNAZ、ADN之间的相互作用。结果表明,CL-20受到PET的促进而提前分解,PBT/CL-20中CL-20的分解峰温比CL-20单组分提前约36℃。PET大分子对DNTF和TNAZ的升华和挥发起到抑制作用,并使其分解放热反应大幅提前,同时,DNTF和TNAZ气相产物对PET的分解也有促进作用。PET和ADN及其凝聚相产物之间的相互作用较小,但ADN的气相产物对PET有一定的影响。     

大椭圆星载轨道预报系统设计

分析了大椭圆星载轨道预报对模型精度的要求,对大椭圆轨道动力学模型进行了合理的简化,比较了多个单步数值迭代算法的优劣,选择了适合大椭圆星载轨道预报要求的单步迭代算法,建立了大椭圆星载轨道预报系统.仿真结果验证了该预报系统的可用性与高效性.     

可变参数AWGN深空信道模型特性分析及其仿真

文章在研究深空通信信道的统计特性的基础上,建立了可变参数AWGN（VPAWGN）模型来模拟深空通信信道,主要考虑噪声功率、多普勒频移和路径损耗等参数对信道特征的影响。进一步在Visual C＋＋环境下搭建VPWAGN模型,并对各参数对信道的影响进行验证。