W型发动机双轴摆动故障的排除

简要介绍了DPF－2型控制系统在W型发动机上的应用，分析了该系统在使用过程中出现的双轴摆动现象，对整个系统的稳定性进行了探讨，采取措施解决了该发动机双轴摆动故障并进行了试验验证。该研究对进一步完善该型发动机的燃油控制系统有一定的参考作用。     

电大尺寸散射体的RCS计算方法研究

为了更加有效的求解电大目标散射计算问题,在避免谐振区效应情况下获得复杂目标的隐身雷达散射截面(RCS)特性,引用混合场积分方程(CFIE),在快速算法的求解迭代过程中采用共轭梯度算法(CG)的收敛技术,能够稳定的求解电大尺寸的RCS。计算和分析了金属球双站RCS和金属立方体双站RCS,并和精确计算、相关参考文献进行了比较,证明了方法的正确性,计算结果稳定,在工程实际上有较大的应用价值。     

陶瓷纤维梯度增强活塞的梯度方程研究

 功能梯度材料零件具有单质材料零件无法比拟的理化性能优势，然而由于材料分布复杂以及对功能梯度材料本身性能研究不充分，使性能分析存在很多困难。论文应用复合材料热性能理论，采用有限元分析软件ADINA，分析陶瓷纤维梯度增强活塞（材料梯度方程的参数不同）的温度分布和应力分布，结果表明陶瓷纤维梯度层可以明显改变活塞温度分布，缓和由于热膨胀系数不匹配，在陶瓷纤维增强层与活塞本体交界处产生的应力。根据计算结果拟合出温度峰值、整体应力峰值和层间应力峰值与方程系数之间的曲线，并加以验证。     

冷热两股气流在圆管内掺混的速度场、温度场与辐射通量场的数值方法

用数值方法求解冷热两股轴对称平行射流在圆管内掺混的流场、温度场和辐射通量场。计算采用一种通用性的数值方法,其特点是强烈地以物理本质为基础,而不仅仅是单纯的数学推导。这样做,能方便地分析和解释计算结果,使之更真实地接近于实际。 通过计算,分析了当引射系数改变时,掺混的流场,温度场和辐射通量场的变化规律,其结果与实验数据比较一致。     

Modelling of the electromagnetic field in the interplanetary space and in the Earth's magnetosphere

A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented. In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the observational data for September 24–26, 1998 magnetic storm (Dst _min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997. This revised version was published online in August 2006 with corrections to the Cover Date.     

高负荷跨声速压气机动静叶干扰下叶片气动负荷研究

通过数值方法模拟了某型高负荷跨声速压气机在工作点的非定常流场，对级内动静叶的气动干扰进行了深入分析。通过气动力和力矩的变化对动静叶干扰下的叶片非定常气动负荷进行了详细的分析，研究了尾迹和势流干扰下叶片气动负荷的变化规律，结合频谱分析进一步认识了气动负荷各周期分量，研究结果有助于对高负荷压气机内动静叶非定常气动干扰的认识。     

突扩后突缩的三维流场计算

根据有关固体火箭发动机装药后端到喷管间的空间特征,对三维突扩后突缩内部流场计算进行了探索和研究。计算中成功地应用了SIMPLE算法解决复杂的三维流场计算问题,并在初场构成、源项离散及松弛系数的选取等方面都进行了调试改进。通过建立计算模型、划分网格、对方程及边界条件离散化和非线性处理,以及线性方程组求解等,计算得到了符合物理规律的数值解,指出了空间涡及二次涡的存在。     

三维侧面突扩燃烧室冷态气流场的数值模拟

本文对四侧30°进气并带有进气管道和尾喷口的突扩燃烧室冷态气流场进行了数值模拟.对这种复杂非规则边界的计算区域,首次采用分段算法进行计算.结果表明:分段算法可以提高网络利用率,缩短机时,消除虚假扩散,提高计算准确度,计算结果与试验结果基本符合.     

大攻角非对称流动的非定常弱扰动控制

 研制了一种新的大攻角细长旋成体非对称涡的主动控制技术, 即在细长旋成体头部施加非定常弱扰动来控制头部非对称背涡。应用七孔探针测量的空间截面流场揭示了非定常控制下非对称涡变成对称涡的流态特征。测力试验研究结果表明该方法不仅能完全消除背涡的非对称性及其产生的侧向力, 并且有效控制攻角范围从30b直到80b。     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.