飞机主操纵系统疲劳试验载荷谱小操纵位移频次问题研究

针对飞机全机主操纵系统疲劳试验载荷谱中小操纵位移频次影响问题进行了分析和讨论,确定了某机全机主操纵系统小操纵位移频次的级别。同时,在原某机全机主操纵系统疲劳试验载荷谱的基础上再次对其小操纵位移频次进行了计算,去掉了这一级别以下对全机主操纵系统疲劳试验无影响的小操纵位移频次,从而完善了主操纵系统疲劳试验载荷谱。另外,对小操纵位移频次问题研究结果在其全机主操纵系统疲劳试验中的实施效果进行了阐述。     

膨胀循环发动机起动过程研究

针对膨胀循环发动机起动过程的计算问题,基于模块化建模方法,研究了各组件的数学和仿真模型,运用Simulink工具箱,编制了针对液体火箭发动机系统起动过程计算所需的各个模块库。在此基础上,对膨胀循环发动机系统的起动过程进行了仿真研究,分析了起动过程的影响因素。     

星载BX1750A芯片抗单粒子翻转性能评估

用软件包和FOM方法分别计算了BX1750A芯片在三种太阳同步轨道以及不同宇宙环境下的单粒子翻转率。根据器件及单片机系统在轨单粒子翻转率与“零翻转”可靠度的关系，量化地评估了该芯片及所属系统应用于不同飞行任务时的抗单粒子翻转(SEU)性能。分析结果表明，BX1750A芯片抗单粒子效应的性能较高，可作为低太阳同步轨道3年或5年寿命卫星关键计算机系统的选用芯片。同时为确保系统SEU零失效，有必要采取软件和其他加固措施。     

FY-1C/D极轨气象卫星及其在轨运行

简要说明了风云一号(FY-1)极轨气象卫星的总体情况。介绍了FY-1C星运行5年。D星运行2年后的测控、电源、热控、敖传、扫描辐射计和星载数据收集与分发(DCDS)分系统、有效载荷空间粒子成分监测器。以及姿控和星载计算机的在轨运行情况。在轨测试结果表明，两星的在轨运行、功能和性能符合任务书的要求。最后总结了长寿命高可靠稳定优质业务运行的FY-1C，D星的创新点、主要成绩，并给出了部分应用情况。     

生态环境材料——社会可持续发展的物质基础

 生态环境材料是近年来在先进材料研究中提出的一个新研究领域。简要介绍了生态环境材料概念的产生、发展及哲学基础,从材料环境协调性评价、材料和物质的再生循环、与生态系统相协调的材料与工程、环境工程材料、与材料科学相关的生态工程等几方面对生态环境材料研究的最新进展进行了评述。     

A Possible Transfer Mechanism for the 11-Year Solar Cycle to the Lower Stratosphere

Observational evidence of the 11-year solar cycle (SC) modulation of stratosphere temperatures and winds from the ERA-40 dataset is reviewed, with emphasis on the Northern winter hemisphere. A frequency modulation of sudden warming events is noted, with warmings occurring earlier in solar minimum periods than in solar maximum periods. The observed interaction between the influence of the SC and the quasi biennial oscillation (QBO) on the frequency of sudden warmings is noted as a possible clue for understanding their mechanism of influence. A possible transfer route for the 11-year solar cycle from the equatorial stratopause region to the lowest part of the stratosphere is proposed, via an influence on sudden warming events and the associated induced meridional circulation. SC and QBO composites of zonal wind anomalies show anomalous wind distributions in the subtropical upper stratosphere in early winter. Mechanistic model experiments are reviewed that demonstrate a sensitivity of sudden warmings to small wind anomalies in this region. Various diagnostics from these experiments are shown, including EP fluxes and their divergence and also the synoptic evolution of the polar vortex, in order to understand the mechanism of the influence. Some recent GCM experiments to investigate the SC/QBO interaction are also described. They simulate reasonably well the observed SC/QBO interaction of sudden warming events and appear to support the hypothesis that tropical/subtropical upper stratospheric wind anomalies are an important influence on the timing of sudden warmings.     

恒温热源条件下实际回热式布雷顿循环的功率密度优化

计人工质与高、低温侧换热器和回热器的热阻损失、压气机和涡轮机中不可逆压缩和膨胀损失及管路系统中的压力损失，用有限时间热力学方法，导出了恒温热源条件下实际回热式布雷顿循环功率密度与压比间的解析式，借助于数值计算，研究了高、低温侧换热器和回热器的热导率分配对最大功率密度的影响。     

不同生命周期项目组合的约束资本预算优化模型及算法

文章给出了约束资本预算优化模型的一般数学表达式.根据詹姆斯*范霍恩的共同生命周期法的理论,提出了一种对不同生命周期项目组合的约束资本预算优化的新算法.通过算例,说明了新算法与原有算法的差别,结果表明新算法考虑了项目的重置,在满足各种约束的前提下,按照净现值指数的大小选择项目组合,从总体上寻优,得到的净现值总和更大,具有更为优化的特征.     

一种基于余数周期的 PRI精确估计算法

针对传统脉冲重复间隔（PRI）分选算法在估计PRI方面存在的不足，提出了一种对PRI周期信号的周期进行精确估计的算法。该算法首先从待分选脉冲序列中提取出属于一部雷达的脉冲样本，然后利用同余方程的余数周期性质对该雷达脉冲序列的PRI进行精确的估计。相对于传统的PRI估计算法，该算法有效地消除了TOA量化误差对PRI估计造成的影响，可以精确地估计出雷达脉冲序列的准确 PRI数值，从而能够更好地满足信号分选算法的处理需求。理论推导及仿真实验均表明了该算法的有效性。     

Time-dependent cosmic ray modulation

Time-dependent cosmic ray modulation is calculated over multiple solar cycles using our well established two-dimensional time-dependent modulation model. Results are compared to Voyager 1, Ulysses and IMP cosmic ray observations to establish compatibility. A time-dependence in the diffusion and drift coefficients, implicitly contained in recent expressions derived by , ,  and , is incorporated into the cosmic ray modulation model. This results in calculations which are compatible with spacecraft observations on a global scale over consecutive solar cycles. This approach compares well to the successful compound approach of Ferreira and Potgieter (2004). For both these approaches the magnetic field magnitude, variance of the field and current sheet tilt angle values observed at Earth are transported time-dependently into the outer heliosphere. However, when results are compared to observations for extreme solar maximum, the computed step-like modulation is not as pronounced as observed. This indicates that some additional merging of these structures into more pronounced modulation barriers along the way is needed.