基于拟平均根数之差的航天器相对导航UKF滤波算法

针对星载雷达数据(距离及其变率、角度及其变率),推导了以相对拟平均根数为状态变量的星间相对导航UKF滤波算法.建立了包含J2一阶长期项摄动的状态转移方程.推导了无奇点的相对拟平均根数与相对位置速度之间的转换矩阵,并分析了坐标变换中被忽略的二阶项的影响,对转换矩阵的精度进行了有效补偿.提出以相对位置速度为直接观测量,设计了具有自调整功能的测量误差协方差阵,避免了建立观测方程时状态量对直接观测量的繁琐偏导计算.仿真结果证明了该算法的有效性.     

复合材料J型加筋壁板制造技术研究

对J型加筋壁板共胶接技术在实际应用中所存在的主要问题进行了研究,着重介绍了R区芯材精确填充、筋条外型模成型、框架式插销垂直定位、共胶接真空袋封装等关键技术的研究情况,并对相关技术的应用进行了深入分析。研究结果表明,在精确计算的基础上,设计制造专用成型模具可实现R区填充芯材的精确制备,有利于提高加筋壁板胶接质量;选用筋条外型模成型工艺,并设计采用框架式插销垂直定位装置,可有效解决J型筋的表面成型质量、筋条尺寸精度、位置精度等问题;使用已硫化橡胶作为维形挡条、制备合适的内型面软模、优化辅助材料铺放方法,可减少表面质量问题,降低架桥、破袋风险。在应用了上述一系列制造技术后,成功制造了满足使用要求的J型加筋壁板复材零件,并初步实现该类型零件的批量化生产。     

C-400地空导弹武器系统性能分析与比较

C-400即将进入战斗值班形成战斗力,它是未来俄罗斯防空导弹体系中的中远程部分.由于俄对其长期保密,外界对它的了解甚少.综合国内外资料对其多个分系统进行了性能初步分析,并与"爱国者"地空导弹武器系统等进行了对比.     

First results of investigating the space environment onboard the Universitetskii-Tatyana satellite

The complex of scientific pay load installed onboard the research and educational Universitetskii-Tatyana microsatellite of Moscow State University is described. The complex is designed to study charged particles in the near-earth space and ultraviolet emissions of the atmosphere. Data of the measurements of charged particle fluxes in the microsatellite orbit are presented, spectra are calculated, and the dynamics of penetration boundaries for protons of solar cosmic rays (SCR) during geomagnetic disturbances in 2005 is investigated. Intensities of the ultraviolet emission are measured in the entire range of variation of the atmospheric irradiation, as well as intensities of auroras in the polar regions of the Northern and Southern hemispheres. The experimental data on flashes of ultraviolet radiation (transient light phenomena in the upper atmosphere) are considered, and some examples of oscillograms of their temporal development and their distribution over geographical coordinates are presented. Original Russian Text ? V.A. Sadovnichy, M.I. Panasyuk, S.Yu. Bobrovnikov, N.N. Vedenkin, N.A. Vlasova, G.K. Garipov, O.R. Grigorian, T.A. Ivanova, V.V. Kalegaev, P.A. Klimov, A.S. Kovtyukh, S.A. Krasotkin, N.V. Kuznetsov, S.N. Kuznetsov, E.A. Muravyeva, I.N. Myagkova, N.N. Pavlov, R.A. Nymmik, V.L. Petrov, M.V. Podzolko, V.V. Radchenko, S.Ya. Reisman, I.A. Rubinshtein, M.O. Riazantseva, E.A. Sigaeva, E.N. Sosnovets, L.I. Starostin, A.V. Sukhanov, V.I. Tulupov, B.A. Khrenov, V.M. Shakhparonov, V.N. Sheveleva, A.V. Shirokov, I.V. Yashin, V.V. Markelov, N.N. Ivanov, V.N. Blinov, O.Yu. Sedykh, V.P. Pinigin, A.P. Papkov, E.S. Levin, V.M. Samkov, N.N. Ignatiev, V.S. Yamnikol, 2007, published in Kosmicheskie Issledovaniya, 2007, vol. 45, No. 4, pp. 291–305.     

近地卫星编队构形保持方法

针对J2摄动和大气摄动导致低轨编队卫星构型破坏的情况,基于高斯摄动方程给出了以平均轨道根数为被控制量的脉冲控制模型。利用法向脉冲调整轨道倾角和升交点赤经偏差,在轨道上2个位置施加径向和切向脉冲调整其余轨道根数偏差从而修正卫星编队构形。最后通过数值仿真验证了算法的简单性、有效性。     

基于J2ME和J2EE应用平台移动电子商务应用模型研究

目的提出了基于J2ME的移动电子商务系统的应用模型,能较好的解决移动电子商务普遍存在的一些关键问题.方法采用J2ME和J2EE技术体系实现移动电子商务系统的应用模型,并提出交易中安全问题的解决方案.结果利用J2ME和XML技术实现移动购物系统解决方案.结论该模型具有较高灵活性、应用性、安全性和高效性.     

J2EE信息系统数据访问层性能监测与优化设计

针对J2EE信息系统开发阶段从性能优化的角度实现了数据访问层的设计和一个简易的性能监测工具.首先在数据访问层设计阶段,兼顾考虑开发效率和性能问题提供专门的数据访问操作方法;利用面向方面编程(AOP,Aspect-Oriented Programming)技术对系统数据库访问操作及性能指标进行监视,帮助开发者在系统调试运行阶段根据SQL语句执行情况发现数据访问过程中影响性能的因素;开发根据具体的情况调整数据访问的源代码,然后对造成系统性能瓶颈的SQL语句进行性能调优,并替换数据访问层中低效的SQL语句,最终达到优化系统数据访问性能的目的.      

Optical/infrared observations unveiling the formation,nature and evolution of High-Mass X-ray Binaries

In this review I first describe the nature of the three kinds of High-Mass X-ray Binaries (HMXBs), accreting through: (i) Be circumstellar disc, (ii) supergiant stellar wind, and (iii) Roche lobe filling supergiants.     

SN 1987A and SN 1993J: Testing stellar evolution theory?

Nearby supernovae like SN 1987A and SN 1993J provide valuable constraints on the late evolution of massive stars. For this purpose, we review evolutionary models for the progenitor of SN 1987A and confront them with five observational/theoretical tests we devised. We show that single-star models (with the possible exception of rapid-rotation models) fail at least two of these tests, while two binary models (accretion and merger models) are consistent with all available constraints. We conclude that it is most likely that the progenitor of SN 1987A had a binary companion, either at the time of the explosion or at least in the not-too-distant past, and that SN 1987A should therefore not be used to calibrate single stellar evolution theory. For SN 1993J, we infer from the presupernova photometry and the early light curve that its progenitor was a 15M star that lost almost all of its hydrogen-rich envelope prior to the supernova. This seems to require that the progenitor underwent stable case C mass transfer. We discuss future observational tests of binary models for both supernovae.     

带环状裂纹圆棒的J积分评价方法

通过有限元解析方法分别研究了轴向或扭转载荷下带环状裂纹圆棒试样的J积分的评价方法。首先模拟计算得到了一系列带有不同深度环状裂纹的中碳钢圆棒试样的载荷-位移关系,然后分别利用单试样的简单评价法和多试样的能量评价法计算J积分值。结果发现,当圆棒试样的裂纹深度足够深或位移足够小时,两种评价方法计算的J积分值相当一致。