GAP/AN推进剂的热分解催化研究

研究了ＧＡＰ／ＡＮ推进剂的燃速与硝酸铵放热分解峰温之间的相关性，硝酸铵的放热分解峰温越低，推进剂的燃速越高。用热分析方法筛选出了ＧＡＰ／ＡＮ推进剂有效的燃速调节剂ＭＯ，它能促进硝酸铵分解过程中质子转移反应，因而使ＧＡＰ／ＡＮ推进剂燃速提高。     

一种新的软件实现PCM/FM码同步的方法

根据PCM/FM信号的特点,提出一种软件提取码同步信号的新方法。该方法使用数字瞬时测频法检测信 号每采样点的频率,根据该频率与中心频率之差提取双边沿信号,并用一个除N记数器,得到完整的码同步信号。文中 给出全数字码同步器原理图、MATLAB仿真的性能曲线图和VC实现的软件流程。     

一种新的硬/软件系统可靠性分析方法

在一种新的软件可靠性分析方法基础上，参考硬件系统的阶段性任务可靠性的建方法，为在对于不可修的计算机系统进行可靠性分析时考虑硬、软件之间复杂的相关作用提出了一套比较全面的解决办法。从而为更准确地评估计算机系统可靠性提供了可能。文中分析了一个飞行控制系统实例。     

两项技术使PCM/FM遥测系统信噪比增益提高9dB

介绍国外采用多符号检测技术和Turbo乘积码技术使PCM/FM遥测系统的信噪比增益提高 9dB的研究结果。简要介绍这两种技术的原理 ,指出Turbo乘积码的工程应用前景     

燃烧室新材料在卫星双组元低推力发动机上的应用

对有代表性、有发展前途的几种新材料进行比较 ,并根据应用新材料的低推力发动机燃烧室的结构特点 ,分析了不同冷却方式对双组元低推力发动机性能损失的影响 ,为双组元低推力发动机燃烧室的材料选择、加工工艺、设计优化提供参考。     

气体浮环动静压混合轴承的特性分析

本文对气体浮环动静压混合轴承的静动态特性进行了研究,并给出计算其高速稳定性的简单方法。理论分析与实验结果表明:环面浅腔二次节流动静压混合型气体浮环轴承的高速稳定性是最佳的。     

β Cephei stars from a photometric point of view

This is an observational review, with an emphasis on photometric data and their interpretation. Two lists are presented, one containing Cephei stars, and the other, Cephei suspects. These lists then serve as a basis for discussing such topics as the location of Cephei stars in the observational and theoretical H-R diagrams, the evolutionary state of these stars, the period-luminosity and period-luminosity-color relations, and observational identification of pulsation modes. The paper also includes references to recent work connected with the theoretical discovery that an opacity mechanism is responsible for the excitation of Cephei-star pulsations. Finally, observational programs for verifying the consequences of this discovery are suggested.Belgian Fund for Scientific Research (NFWO).     

惯性/图像组合导航中的双模态双滤波器研究

在简要介绍了飞行器视觉图像定位导航原理及模型的基础上，针对其非线性模型的推广Kalman滤波的收敛与初始条件有关的问题，将其定位导航的两种模型（线性与非线性模型）组合，提出了双模态双滤波器滤波方法。这种滤波能很好地解决非线性推广Kalman滤波的收敛问题。通过第一个线性滤波器的滤波估计给第二个非线性滤波器提供滤波初值，使这一非线性滤波收敛，并能取得较高的滤波精度。     

红外／紫外双色制导系统数学模型及数字仿真

介绍了便携式防空导弹双色导引头中所采用的数字式控制系统代替传统的模拟式控制系统的方法。对导引头和自动驾驶仪部分的数学模型作了简化，并作了全弹道数字仿真。仿真结果表明，该双色制导体系设计方便，抗干扰能力强等。     

Statistical characteristics of locally generated ESF during equinoctial months over Sanya

Understanding the local generation rate of equatorial spread-F (ESF) is important for forecasting ionospheric scintillation. Using the GPS ionospheric scintillation/TEC and VHF radar data during March-April and September-October from 2010 to 2014, the occurrence of ionospheric scintillation, TEC fast fluctuation, and backscatter plume were studied. Through analyzing the simultaneous occurrence of ionospheric scintillation, TEC fast fluctuation and backscatter plume, the local generation rate of ESF over Sanya was investigated. The results show that the monthly generation rate varies between 0% and 68%. A significant equinoctial asymmetry of local generation rate of ESF can be found in 2010, 2013 and 2014. The local generation rate of ESF increases from 2010 to 2014 during March-April, while it does not have similar trend during September-October. The plasma vertical drift influenced by solar activity has a significant impact on the monthly generation rate. The equinoctial asymmetry of plasma vertical drift may contribute a lot to the equinoctial asymmetry of the generation rate of ESF.