攻击机对防空雷达的首攻概率研究

通过分析攻击机的辐射源定位/攻击过程,研究了攻击机水平轰炸防空雷达的首攻概率。首先分析了攻击机发现目标过程,并给出了相应的发现目标概率计算模型;其次,具体分析了攻击机水平轰炸防空雷达的进入目标过程,并给出相应的进入目标概率计算模型;最后,通过相关示例对模型中的主要因素进行了分析,证实了模型的有效性。     

基于B样条曲线的无人机航路规划算法

提出了一种动态环境中无人机(UAV)航路规划与重规划算法。根据战场中各个已知威胁的位置建立可行点之间的有向图，用Dijkstra算法生成一条由若干直线段连接的参考航路，再利用B样条曲线具有C^2连续性、局部性、保凸性以及B样条曲线的曲率变化比较均匀的特点，对规划的参考航路进行修正和验证，使得规划航路对无人机安全可飞。当遇到突然出现的威胁时，可对航路进行局部重规划。     

雷达舰船目标回波建模研究

阐述了根据电磁波几何绕射理论所建立的舰船目标雷达回波模型,利用该模型可产生多种假设目标的回波数据,用于弥补科研试验过程中所需的多种条件下的雷达目标回波数据,所建模型在实际试验中得到了较好的应用.     

某型航空发动机环形燃烧室振动特性分析

建立了环形燃烧室薄壁多孔结构的有限元模型,模拟燃烧室在实际工作中的安装条件,分析了燃烧室在不同工作状态下的模态频率和模态振型等.利用常温自由状态条件下有限元模型计算的振动特性,与该状态下的试验结果进行对比,修正计算模型.结果表明,修正后的计算结果与试验结果基本相符,保证了环形燃烧室各工作状态下振动特性分析的有效性.研究了不同工作状态对燃烧室温度场的影响及温度场对燃烧室模态频率的影响,结果表明燃烧室的工作温度越高,其模态频率越低;另外,计算结果表明该近似对称结构系统具有非单构系统的特点,其相似振型可作为同一阶振型加以考虑.     

提高基建档案管理水平的方法及措施

高校基本建设档案管理,是高校进行整体规划和科学管理的重要组成部分。基于基建档案的内容特点和主要作用,将高校发展建设中基建档案的管理方法及措施进行一些探讨。要充分发挥基建档案作用,必须保证基建档案的数量和质量,使其具有完整性、准确性、系统性和安全性。应采取的方法及措施是：提高基建档案立卷部门的归档意识,建立优质基建档案;档案管理部门应加强档案文件材料的质量检查,强化基建档案的验收工作;提高档案人员的管理水平,改进基建档案的利用及保护方式。     

端壁抽吸位置对压气机叶栅角区分离控制的影响

以某高负荷压气机叶栅为研究对象,应用数值模拟方法探索了叶栅端壁不同抽吸位置对角区流动结构、通道漩涡发展过程以及叶栅性能的影响规律,寻求控制角区分离的可行方法。研究结果表明:在叶栅前缘上游5%C(弦长)位置实施抽吸,延缓了通道涡的形成,但导致叶栅来流攻角发生改变,在角区形成角区分离涡,并且该漩涡与通道涡相互促进,进一步恶化叶栅流场,导致叶栅落后角增大,损失增加;在叶栅通道激波后25%C端壁抽吸,吸除了上游端壁积累的高熵低能气流,制约了通道涡的迅速发展,改善了叶栅通道的流场结构,降低了流动损失,但并未对上游流场产生较大影响,是一种可行的方案。然而25%C处抽吸后,未能完全消除分离,在端部与叶栅通道主流之间存在较高损失区域。     

脉冲等离子体推力器放电波形设计评估仿真研究

运用磁流体动力学的方法,对脉冲等离子体推力器推力室工作过程开展三维双温MHD数值仿真,并开展对推力室的工作机理的分析研究。通过该模型计算得到的推进剂烧蚀质量和元冲量与实验结果相符,同时针对不同初始电压、电容以及两种特征波形的情况进行评估,为推力器的放电波形设计提供指导依据。结果显示在推力器波形设计的初期,是采用电流高变化率低能量水平,还是采用电流低变化率高能量水平,需要结合实际,进行优化评估。     

N2O/C3H8火炬式点火器试验研究

为了研究氧化亚氮/丙烷的点火特性,在理论分析的基础上采用电激励火炬式点火方案并组建了实验系统,在不同的流量和余氧系数工况下进行了N2O(g)/C3H8(g),N2O(g)/C3H8(l)点火特性实验。结果表明:采用气液同轴离心式喷嘴的电激励火炬式点火方案可行,实现了低余氧系数下的点火。所设计的点火器在1J的点火能量下,N2O(g)/C3H8(g)在燃烧室压强为环境大气压条件下的成功点火余氧范围为0.222～0.321;N2O(g)/C3H8(l)在燃烧室平衡压强为0.50～0.65 MPa时成功点火余氧范围为0.299～0.407,并在平衡压强提高至1～1.3 MPa后成功地引燃主发动机。     

The Magnetic Field of Mercury

The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and observationally to distinguish the internal field from that due to the solar wind interaction. Conversely, the small field also means that Mercury offers an important opportunity to advance our understanding both of planetary magnetic field generation and magnetosphere-solar wind interactions. The observations from the Mariner 10 magnetometer in 1974 and 1975, and the MESSENGER Magnetometer and plasma instruments during the probe’s first two flybys of Mercury on 14 January and 6 October 2008, provide the basis for our current knowledge of the internal field. The external field arising from the interaction of the magnetosphere with the solar wind is more prominent near Mercury than for any other magnetized planet in the Solar System, and particular attention is therefore paid to indications in the observations of deficiencies in our understanding of the external field. The second MESSENGER flyby occurred over the opposite hemisphere from the other flybys, and these newest data constrain the tilt of the planetary moment from the planet’s spin axis to be less than 5°. Considered as a dipole field, the moment is in the range 240 to 270 nT-R _M ³ , where R _M is Mercury’s radius. Multipole solutions for the planetary field yield a smaller dipole term, 180 to 220 nT-R _M ³ , and higher-order terms that together yield an equatorial surface field from 250 to 290 nT. From the spatial distribution of the fit residuals, the equatorial data are seen to reflect a weaker northward field and a strongly radial field, neither of which can be explained by a centered-dipole matched to the field measured near the pole by Mariner 10. This disparity is a major factor controlling the higher-order terms in the multipole solutions. The residuals are not largest close to the planet, and when considered in magnetospheric coordinates the residuals indicate the presence of a cross-tail current extending to within 0.5R _M altitude on the nightside. A near-tail current with a density of 0.1 μA/m² could account for the low field intensities recorded near the equator. In addition, the MESSENGER flybys include the first plasma observations from Mercury and demonstrate that solar wind plasma is present at low altitudes, below 500 km. Although we can be confident in the dipole-only moment estimates, the data in hand remain subject to ambiguities for distinguishing internal from external contributions. The anticipated observations from orbit at Mercury, first from MESSENGER beginning in March 2011 and later from the dual-spacecraft BepiColombo mission, will be essential to elucidate the higher-order structure in the magnetic field of Mercury that will reveal the telltale signatures of the physics responsible for its generation.     

离心压气机内不同非定常源影响实验研究

使用热线风速仪对扩压器内的非定常流场进行了测量,采用锁相采样—集平均技术对热膜测量的瞬时信号进行了处理,对离心压气机内扩压器势反冲效应和叶轮尾流的非定常影响进行了分离,采用＂逆频谱分析＂方法求解了不确定性非定常性,研究了离心压气机内不同非定常源的影响。结果表明,扩压器的势反冲效应同叶轮叶片的非定常影响处于同一数量级,扩压器的势反冲效应略小一些。扩压器的势反冲效应同叶轮叶片的非定常影响均是沿流向不断减小,且二者之间的差距沿流向也不断减小。叶轮叶片的非定常影响对扩压器叶片的位置较为敏感,靠近扩压器凸面侧的测点受叶轮叶片的非定常影响较大。径向间隙内不确定非定常度受扩压器叶片的反冲影响较大。