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。     

某型直升机旋翼转速表的数字化设计方案

提出某型直升机数字旋翼转速表的研制方案,给出以频率/数字(F/D)变换电路为核心的主要硬件原理,分析了采样误差的产生及抑制误差的措施.装机部件研制成功证实了方案的可行性.     

直升机桨叶耐颗粒物/砂磨蚀标准分析

在分析研究直升机桨叶耐颗粒物/砂磨蚀标准主要技术要素的基础上,全面对比分析了MIL-STD-3033、ГОСТР52560-2006、GJB 1171-1991等国内外标准的基本内容,提出了装备研制及标准化工作相关建议。     

Plasmaspheric electron content derived from GPS TEC and FORMOSAT-3/COSMIC measurements: Solar minimum condition

The plasmaspheric electron content (PEC) was estimated by comparison of GPS TEC observations and FORMOSAT-3/COSMIC radio occultation measurements at the extended solar minimum of cycle 23/24. Results are retrieved for different seasons (equinoxes and solstices) of the year 2009. COSMIC-derived electron density profiles were integrated up to the height of 700 km in order to retrieve estimates of ionospheric electron content (IEC). Global maps of monthly median values of COSMIC IEC were constructed by use of spherical harmonics expansion. The comparison between two independent measurements was performed by analysis of the global distribution of electron content estimates, as well as by selection specific points corresponded to mid-latitudes of Northern America, Europe, Asia and the Southern Hemisphere. The analysis found that both kinds of observations show rather similar diurnal behavior during all seasons, certainly with GPS TEC estimates larger than corresponded COSMIC IEC values. It was shown that during daytime both GPS TEC and COSMIC IEC values were generally lower at winter than in summer solstice practically over all specific points. The estimates of PEC (h > 700 km) were obtained as a difference between GPS TEC and COSMIC IEC values. Results of comparative study revealed that for mid-latitudinal points PEC estimates varied weakly with the time of a day and reached the value of several TECU for the condition of solar minimum. Percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 50–60%) during night-time and lesser values (25–45%) during day-time.