滚动轴承疲劳强度分布计算

根据P－S－N曲线上疲劳寿命存活率和疲劳强度存活率的等同性原理，借助已知的给定载荷下疲劳寿命概率密度函数，计算出未知的给定寿命下疲劳强度概率密度函数，进一步进行可靠性分析奠定基础。     

利用光学层析技术重构超声速绕流流场密度分布

在连续式风洞中,采用单光路旋转流场干涉测量和计算机层析方法获得了含模型的超声速绕流流场密度分布.首先利用多种图像处理方法,并引入计算机辅助功能,对干涉图片进行精确判读和定量处理,准确重构波前相位信息;获得了相应的PV值、RMS值以及前15阶的Zernike多项式系数;通过同原始CFD模型波前数据的对比,系统的重构精度RMS优于λ/10.在获得一系列单帧干涉波前相位数据的基础上,采用光学层析技术,设计计算机迭代算法,构造内部旋转矩阵,重构了超声速绕流流场密度分布,可以非常直观地获得待测流场不同方向截面上的密度分布状况.     

GEO轨道兆瓦级空间太阳能电站接收整流技术研究

依据中国空间太阳能电站建设中远期规划和技术发展水平,预估兆瓦级电站发射天线口径为200 m左右,并根据收发天线口径尺寸的约束关系以与接收天线口径相关的波束收集效率和构建成本之间的矛盾为问题导向,通过研究不同口径的接收天线口面上功率密度分布,分析与之匹配的后端整流电路需求,给出了接收天线口径的优选过程。研究结果表明5 km为较合理的兆瓦级电站接收天线设计建设指标,且在整个接收整流阵列中仅需同一种整流器件,同样整流电路即可实现较高的整流效率,为实现兆瓦级空间太阳能电站（Space solar power satellite,SSPS）的演示验证系统论证提供了技术支撑。最后以此为基础研究了整流电路的设计实现,给出了适用于较低输入功率密度下提高整流效率的技术途径。     

基于矩阵变压器的1 MHz GaN LLC谐振变换器

现代工业生产越来越重视节约能源和降低成本,促使高效率和高功率密度成为分布式电源系统发展的主要方向。随着信息技术、计算机系统和电动汽车等领域的发展,对具有高效率、高功率密度的隔离电源的需求显著增加。本文针对数据中心服务器电源对高效率、高功率密度的需求,通过提升开关频率到1 MHz来提高变换器的功率密度;并对传统LLC变换器进行研究,阐述其工作原理及相对其他变换器的优势。在此基础上,应用GaN器件、矩阵变压器和同步整流来进一步优化传统LLC谐振变换器;最后设计并制作了一台1kW,380V输入、12V输出实验样机,功率密度达到300W/in3,验证了理论分析的正确性。     

弹体脉动压力特征的实验研究

针对弹体模型进行了表面脉动压力特性实验研究,实验马赫数M∞=0. 8、0. 84、0. 86、0. 92、1. 0、1. 15、2. 0、2. 5,实验迎角α=-5°、-3°,0°、3°、5°,沿弹体轴向测量了14个特征点的脉动压力,得到了弹体表面测点的脉动压力系数、频谱曲线以及相关性系数等实验数据.结果表明:脉动压力系数总体上随马赫数增加而降低.不同马赫数.迎角α=0°的条件下沿轴向各测点压力脉动之间的空间相关性有类似的分布规律,且各测点脉动压力基本互不相关.在实验的迎角下,脉动压力系数在弹体表面曲率变化较小的位置基本上不随来流迎角的改变而变化,膨胀拐角肩部位置的脉动压力系数随着迎角的改变而变化较大.超声速来流的功率谱能量峰值所对应的主频出现明显的低频特征;跨音速来流时特征频率随着马赫数的增加而增大,功率谱能量峰值位于特征频率处.     

基本随机变量的重要性测度及其概率密度演化算法

为进一步完善当前的基本变量的重要性分析,在单一的矩独立的重要性测度指标的基础上,建立了一个新的矩独立的重要性测度指标体系,该体系包括基本变量的总重要性测度、平均总重要性测度、主重要性测度和平均主重要性测度,用以衡量不同要求下基本随机变量对系统或模型输出响应整体不确定性的影响程度.给出了各个重要性测度指标的定义,分析了各个重要性测度指标的工程意义和适用范围.结合概率密度演化方法高效、准确的优点,提出了一种基于概率密度演化方法的重要性测度求解方法.文中算例证明:所提指标体系相比当前指标体系更加全面合理,所提方法能在高精度求得各重要性测度结果的基础上大幅提高计算效率.     

含晶界单层过渡金属硫化物的压电效应研究

在单层过渡金属硫化物（Transition metal dichalcogenides,TMDs）的合成过程中,缺陷是不可避免的,而且缺陷对单层TMDs的物理化学性质有着重要的影响。为了研究晶界（Grain boundaries,GBs）对单层TMDs压电效应的影响,基于密度泛函理论（Density functional theory,DFT）,计算了36种含晶界单层TMDs和36种不含晶界单层TMDs的压电系数。结果表明：晶界的存在会增强单层TMDs的压电效应,这是由于晶界会导致体系产生应变梯度,从而激发了挠曲电效应。压电系数的变化呈现明显的周期趋势,即随着硫族元素相对原子质量的增加压电系数逐渐增大,其中,含晶界的单层MoTe₂的压电系数最大为11.17 pm/V,与单层MoTe₂ （8.74 pm/V）相比,提高了约27.8%。本文的研究结果可以为开发应用于飞行器中的高灵敏度传感器和高精度控制器的设计提供理论指导。     

Orbital reference frame estimation with power spectral density constraints for drag-free satellites

The drag-free satellites are widely used in the field of fundamental science as they enable the high-precision measurement in pure gravity fields. This paper investigates the estimation of local orbital reference frame (LORF) for drag-free satellites. An approach, taking account of the combi-nation of the minimum estimation error and power spectral density (PSD) constraint in frequency domain, is proposed. Firstly, the relationship between eigenvalues of estimator and transfer func-tion is built to analyze the suppression and amplification effect on input signals and obtain the eigenvalue range. Secondly, an optimization model for state estimator design with minimum estima-tion error in time domain and PSD constraint in frequency domain is established. It is solved by the sequential quadratic programming (SQP) algorithm. Finally, the orbital reference frame estimation of low-earth-orbit satellite is taken as an example, and the estimator of minimum variance with PSD constraint is designed and analyzed using the method proposed in this paper.     

Depth dependency of neutron density produced by cosmic rays in the lunar subsurface

Depth dependency of neutrons produced by cosmic rays (CRs) in the lunar subsurface was estimated using the three-dimensional Monte Carlo particle and heavy ion transport simulation code, PHITS, incorporating the latest high energy nuclear data, JENDL/HE-2007. The PHITS simulations of equilibrium neutron density profiles in the lunar subsurface were compared with the measurement by Apollo 17 Lunar Neutron Probe Experiment (LNPE). Our calculations reproduced the LNPE data except for the 350–400 mg/cm² region under the improved condition using the CR spectra model based on the latest observations, well-tested nuclear interaction models with systematic cross section data, and JENDL/HE-2007.     

The asymmetrical features in electron density during extreme solar minimum

The variations of plasma density in topside ionosphere during 23rd/24th solar cycle minimum attract more attentions in recently years. In this analysis, we use the data of electron density (Ne) from DEMETER (Detection of Electromagnetic Emissions Transmitted from Earthquake Regions) satellite at the altitude of 660–710 km to investigate the solstitial and equinoctial asymmetry under geomagnetic coordinate system at LT (local time) 1030 and 2230 during 2005–2010, especially in solar minimum years of 2008–2009. The results reveal that ΔNe (December–June) is always positive over Southern Hemisphere and negative over northern part whatever at LT 1030 or 2230, only at 0–10°N the winter anomaly occurs with ΔNe (December–June) > 0, and its amplitude becomes smaller with the declining of solar flux from 2005 to 2009. The ΔNe between September and March is completely negative during 2005–2008, but in 2009, it turns to be positive at latitudes of 20°S–40°N at LT 1030 and 10°S–20°N at LT 2230. Furthermore, the solstitial and equinoctial asymmetry index (AI) are calculated and studied respectively, which all depends on local time, latitude and longitude. The notable differences occur at higher latitudes in solar minimum year of 2009 with those in 2005–2008. The equinoctial AI at LT 2230 is quite consistent with the variational trend of solar flux with the lowest absolute AI occurring in 2009, the extreme solar minimum, but the solstitial AI exhibits abnormal enhancement during 2008 and 2009 with bigger AI than those in 2005–2007. Compared with the neutral compositions at 500 km altitude, it illustrates that [O/N₂] and [O] play some roles in daytime and nighttime asymmetry of Ne at topside ionosphere.