多种失效模式相关的机构运动可靠度计算方法

机构运动中必然存在多种相关失效模式,多为影响机构运动的各类随机变量函数.为了在机构运动可靠性分析中有效考虑多种相关失效模式的影响,建立了考虑多种失效模式相关条件下的机构运动可靠度计算模型,并实现了对多种失效模式相关条件下的机构运动可靠度计算模型的求解,为考虑多种相关失效模式下的机构运动可靠性分析提供了一种有效途径.以6408滚动轴承为例,进行100 000抽样计算,考虑失效模式相关条件下运动可靠度为95.998 9%.该方法精度较高,具有一定的理论意义和应用价值.     

扇区繁忙时段交通流的不均衡度量化研究

以容流量及拥挤度等指标进行的空中交通运行评价无法全面反映空中交通的实际运行状况.在依据重要点对航路段进行分组的基础上,通过计算超容比,确定了扇区繁忙时段,基于多项式二次拟合分析了超容比与基尼系数以及泰尔指数之间的数量关系,基于3σ原则确定了不同超容比情况下的理想不均衡度的取值范围.应用方法对厦门1号扇区的实际运行数据进行了计算分析,验证了不均衡度量化方法的适用性.     

域k上三次一般方程式的解的计算

我们已经研究了域k上的n（n≥5）次一般方程在特征标为0的情形下关于幂根是不可解的，而对于n≤4是可解的。本文利用n次循环域的拉格朗日分解式及循环群σ∈G（K/k）的结构，推出域k上的三次一般方程在特征标为0的情形下一般解的计算公式。     

对航天职工薪酬满意度调查的分析

本文介绍了航天某军民结合型研究所现行的薪酬结构和分配办法,通过对单位员工的薪酬满意度调查,分析该薪酬结构的特点与不足,为下一步的薪酬设计奠定基础。     

论信息产业就业总量的核算方法

21世纪是知识经济的时代，知识经济最活跃的生产部门是那些广泛应用高新技术的新兴产业，信息产业是首当其冲的一个。信息产业的竞争追本溯源是知识与技术的竞争，也就是人才的竞争。因而人力资本核算在信息产业核算研究中有着重要的理论和现实意义，本文在说明有关统计指标的基础上，就信息产业的就业总量中纯信息部门就业总量核算、混合信息部门就业总量核算以及整个信息部门就业核算这几个方面进行了核算方法的研究。     

一种膨胀映射的不动点定理

王尚志给出了若干种膨胀映射的概念，并证明了它们的不动点存在定理。对其中第一型膨胀映射的不动点定理做了进一步推广。     

正态分位点的矩阵算法浅析

假设标准正态的t分位点记为z(t),本文将根据z(t)的Taylor展开式中各个系数之间的矩阵递推关系,给出一种计算z(t)的近似值的方法,并给出具体的程序运算来验证本文的结论.     

高垂直度和低沉积的MEMS陀螺梳齿结构释放工艺

梳齿型微机电系统（MEMS）陀螺的释放要求结构具有垂直度高、释放过程沉积聚合物少的特点,通过优化深硅刻蚀的工艺参数,包括钝化气体八氟环丁烷（C4F8）的流量、衬底温度、刻蚀气体六氟化硫（SF6）的流量和钝化气体C4F8的压力,实现了结构垂直度为90.0°、支撑层表面沉积物厚度为87.1nm的梳齿结构释放工艺。深硅刻蚀工艺的优化为高性能MEMS陀螺的加工提供了基础。     

Analysis of the data processing strategies of spherical harmonic expansion model on global ionosphere mapping for moderate solar activity

Spherical harmonic (SH) expansion is widely used to model the global ionosphere map (GIM) of vertical total electron content (VTEC). According to the impact of different data processing methods of the SH expansion model on the VTEC maps, we specifically performed comprehensive analysis in terms of the data sampling rate, the time resolution, the spherical harmonic degree, and the relative constraint. One month of GPS data (January in 2016) from the International GNSS (Global Navigation Satellite System) Service (IGS) network in a moderate ionospheric activity period at the descending phase of Solar Cycle 24 was processed. To improve the computational efficiency of the daily GIM generation, the data sampling rate of 5?min was recommended allowing the GIM precision loss within 0.10 TECU (total electron content unit). The global VTEC map could be better represented in temporal and spatial domains with higher time resolution and higher spherical harmonic degree, especially at low latitude bands and in the southern hemisphere. The GIM precision improvement was about 10.91% for 1-h and about 15.15% for 0.5-h compared with the commonly used 2-h time resolution. The use of spherical harmonic degree 17 or 20 instead of 15 could improve the precision by 3.19% or 6.06%. We also found that an optimal relative constraint had to be found experimentally considering both the GIM precision and the GIM root mean square (RMS) map.     

Stability of relative equilibria of the full spacecraft dynamics around an asteroid with orbit–attitude coupling

The full dynamics of spacecraft around an asteroid, in which the spacecraft is considered as a rigid body and the gravitational orbit–attitude coupling is taken into account, is of great value and interest in the precise theories of the motion. The spectral stability of the classical relative equilibria of the full spacecraft dynamics around an asteroid is studied with the method of geometric mechanics. The stability conditions are given explicitly based on the characteristic equation of the linear system matrix. It is found that the linearized system decouples into two entirely independent subsystems, which correspond to the motions within and outside the equatorial plane of the asteroid respectively. The system parameters are divided into three groups that describe the traditional stationary orbit stability, the significance of the orbit–attitude coupling and the mass distribution of the spacecraft respectively. The spectral stability of the relative equilibria is investigated numerically with respect to the three groups of system parameters. The relations between the full spacecraft dynamics and the traditional spacecraft dynamics, as well as the effect of the orbit–attitude coupling, are assessed. We find that when the orbit–attitude coupling is strong, the mass distribution of the spacecraft dominates the stability of the relative equilibria; whereas when the orbit–attitude coupling is weak, both the mass distribution and the traditional stationary orbit stability have significant effects on the stability. We also give a criterion to determine whether the orbit–attitude coupling needs to be considered.