面向深空时变信道的数据传输策略

将呈现随机“好”、“坏”状态跳变的深空Ka频段链路噪声温度建模为两状态Gilbert-Elliot信道,考虑深空下行发送端只能获得延迟的信道状态信息（CSI）的限制,结合部分观测马尔科夫决策理论设计了基于延迟CSI预测信道状态的自适应最大化吞吐量传输策略。理论推导了在深空通信环境下最优传输策略的关键阈值,并给出了简化的闭合解计算式。通过地球-火星通信参数仿真,校验了该方案能有效提高吞吐量,提高文件传输效率。     

二氧化氮催化硝化甘油分解机理的数值计算

采用密度泛函理论（DFT）在B3LYP/6-31+G（d,p）水平上模拟计算了NO₂对硝化甘油（NG）催化分解的反应机理。通过与O—NO₂均裂、HNO₂分子内消去反应对比发现,NO₂分子对NG分解反应有显著的催化效应;NG的催化分解途径有α-H夺氢催化和β-H夺氢催化,计算得出2种途径的反应能垒分别为105.337 k J/mol和124.381 k J/mol,说明α-H夺氢催化更容易发生。     

一种无人机旋翼设计方法

为了提高多旋翼无人机的航时,本文提出了一种无人机旋翼设计方法.该方法根据给定的爬升速度、旋翼转速、拉力、旋翼直径、桨叶数、翼型,能够计算出最大力效旋翼的几何特性,包括弦长分布、桨叶角分布.利用该方法设计了某型无人机的旋翼,得到了桨叶角和弦长沿径向的分布.制作了旋翼模型,并且开展了旋翼台架试验.在不同转速下,测量出拉力、...     

Research on failure criterion of composite based on unified macro- and micro-mechanical model

A new unified macro- and micro-mechanics failure analysis method for composite structures was developed in order to take the effects of composite micro structure into consideration. In this method, the macro stress distribution of composite structure was calculated by commercial finite element analysis software. According to the macro stress distribution, the damage point was searched and the micro-stress distribution was calculated by reformulated finite-volume direct averaging micromechanics (FVDAM), which was a multi-scale finite element method for composite. The micro structure failure modes were estimated with the failure strength of constituents. A unidirectional composite plate with a circular hole in the center under two kinds of loads was analyzed with the traditional macro-mechanical failure analysis method and the unified macro- and micro-mechanics failure analysis method. The results obtained by the two methods are consistent, which show this new method’s accuracy and efficiency.     

Si3 N4 粉体的分散及表面改性

研究了以聚丙烯酸铵为分散剂的Si3N4悬浮体的分散特性,以及酸洗和热氧化两种表面改性方法对Si3N4悬浮体的分散性和流变特性的影响.结果表明:分散剂聚丙烯酸铵的最佳酸碱环境为pH=9,最佳使用含量为0.2wt％,酸洗可有效去除粉料中的金属杂质,使Si3N4粉体在悬浮体中粒径分布更集中且粒径主峰值向小粒径移动,同时可使悬浮体的黏度降低.热氧化处理可大幅度降低Si3N4悬浮体的黏度,提高其流变特性.     

Solar Wind Turbulence and the Role of Ion Instabilities

Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In addition to the presence of magnetic field, the differences with neutral fluid isotropic turbulence are: (i) weakness of collisional dissipation and (ii) presence of several characteristic space and time scales. In this paper we discuss observational properties of solar wind turbulence in a large range from the MHD to the electron scales. At MHD scales, within the inertial range, turbulence cascade of magnetic fluctuations develops mostly in the plane perpendicular to the mean field, with the Kolmogorov scaling $k_{\perp}^{-5/3}$ for the perpendicular cascade and $k_{\|}^{-2}$ for the parallel one. Solar wind turbulence is compressible in nature: density fluctuations at MHD scales have the Kolmogorov spectrum. Velocity fluctuations do not follow magnetic field ones: their spectrum is a power-law with a ?3/2 spectral index. Probability distribution functions of different plasma parameters are not Gaussian, indicating presence of intermittency. At the moment there is no global model taking into account all these observed properties of the inertial range. At ion scales, turbulent spectra have a break, compressibility increases and the density fluctuation spectrum has a local flattening. Around ion scales, magnetic spectra are variable and ion instabilities occur as a function of the local plasma parameters. Between ion and electron scales, a small scale turbulent cascade seems to be established. It is characterized by a well defined power-law spectrum in magnetic and density fluctuations with a spectral index close to ?2.8. Approaching electron scales, the fluctuations are no more self-similar: an exponential cut-off is usually observed (for time intervals without quasi-parallel whistlers) indicating an onset of dissipation. The small scale inertial range between ion and electron scales and the electron dissipation range can be together described by $\sim k_{\perp}^{-\alpha}\exp(-k_{\perp}\ell_{d})$ , with α?8/3 and the dissipation scale ? _d close to the electron Larmor radius ? _d ?ρ _e . The nature of this small scale cascade and a possible dissipation mechanism are still under debate.     

民用涡扇发动机预测控制器设计

对一定包线范围内的稳态预测控制器和加速减速过渡态控制器设计展开研究.针对某大涵道比民用涡扇发动机,根据发动机进口参数的相对变化指标对控制区域进行划分,以标称点处发动机线性模型为对象设计了相应的预测控制器,利用提出的多层参数调度方案实现了不同飞行条件及不同发动机状态下预测控制器参数的自适应调整.仿真结果表明:所设计的发动机预测控制系统在控制区域内的设计点和非设计点均具有良好的性能,为全包线设计提供了有效方法.     

民用飞机最小离地速度试飞实施方法研究

对民用飞机最小离地速度( VMU )试飞实施方法进行了研究,主要包含了条款的理解、试验准备、试验分工、模拟器工作准备、试飞技术和数据处理等内容,为民用飞机最小离地速度试飞提供指导。同时作为国内新兴的职业---试飞工程师( FTE),也对其在试飞过程中的分工和职责进行了阐述。     

任意曲面上射线的寻迹方法

为计算任意曲面上天线间的隔离度,提出一种射线寻迹的新算法——最小夹角法.首先对任意曲面表面进行三角形网格剖分,并按照文中要求的格式生成模型表面网格数据;用文中提出的"最小夹角法"对上述网格数据进行处理,从而达到快速准确地找出任意曲面上、任意两点间的短程线.求解了位于圆柱体、椭球体及任意组合体上任意两点间的短程线长度,验证了"最小夹角法"的准确性.     

基于某微型发动机对比分析轴流涡轮与向心涡轮的气动性能与减重

为了确定厘米级微型涡轮发动机在相对较大功率、流量需求时的涡轮形式,以实现发动机更高的性能,本文基于某直径12厘米微发样机开展研究。本文估算了该样机整机环境下单级轴流涡轮的做功能力,并按参数优选规律设计了一台微型轴流涡轮,将之与该样机所采用的微型向心涡轮进行对比,基于CFD和CAD工具分析了两种叶轮在功率、效率及尺寸重量方面的差别。研究表明：在先进微小型发动机总压比提高（4～6,本文设计采用4.2）的情况下,涡轮为了在保持效率的同时满足压气机更高的功率需求,轴流式必须采用双级方案,向心式单级就可满足要求;在压气机压比4～6条件下,进一步对比双级轴流与单级向心方案的结果显示,当流量小于500g/s时,向心式具有尺寸重量优势,发动机能实现较高的推重比。针对厘米级微型发动机,在发动机增压比较高且没有超出单级向心涡轮做功能力的范围时,向心涡轮方案是更好的选择。