一种新型电解电源设计及其实验研究

从电解电源的高频高效化、绿色化、数字化及智能化的发展方向出发,利用电流增强原理,设计了一种开关管带并联辅助网络的零电压全桥软开关电路拓扑,具有节能增效、可靠性高的优点.采用TMS320LF 2407A为核心控制芯片.得到了全桥移相PWM输出波形,并设计了反馈信号调理电路与后端驱动电路,电路形式简单紧凑,实现了软开关电解电源的全数字化控制.     

铝阳极在KOH甲醇-乙醇体系中的电化学性能

为了提高铝的活化性能以及降低铝的腐蚀,用电化学方法研究了在碱性甲醇-乙醇有机体系中,添加剂H2O对铝阳极(99.999%)电化学行为的影响。结果表明:4 mol/L KOH+甲醇-乙醇(5∶5)+30%H2O体系能大幅度抑制铝腐蚀,缓蚀率高达70.04%,但极化程度有所增大。在-1.20 V处,铝的电流密度高达72.66 mA/cm2;开路电位Eocp负移程度最大(-1.933 V)。     

航天铝基复合材料零部件超精密加工技术研究

针对航天高碳化硅铝基复合材料零部件采用聚晶金刚石PCD刀具进行了超精密车削加工试验，用原子力显微镜AFM和扫描电子显微镜对其进行了检测，分析了零部件表面粗糙度值的大小及影响因素、SiCw变形破坏机理、已加工表面微观结构及加工变质层特性。结果表明，超精密车削高碳化硅铝基复合材料零部件可以获得超精密级加工表面（如Ra11．5nm）；超精密车削过程中SiC，存在着三种主要变形破坏机理：直接剪断型、拔出型和压入型，且以直接剪断型为主。直接剪断的SiCw对表面粗糙度值影响最小，而后二者是影响表面粗糙度值达到超精密级的主要障碍；超精密加工零部件表面仍会产生很薄的加工变质层。     

电子设备可靠性预计参数综合分析方法研究

如何调整元器件的参数以满足可靠性要求并达到最佳的效费比?传统的方法是绘制故障率随单个预计参数变化的曲线，然后根据变化的趋势分别进行调整，但该方法很难直观地反映出多参数对故障率的综合影响，为了达到优化的目的，设计人员需要根据经验反复地调整各类参数。为此，本文结合电子产品可靠性预计软件，给出了直观分析各参数对电子设备可靠性预计结果综合影响的方法。     

涡轴发动机发展与技术趋势

首先,对美国20世纪70年代以来各时期涡轴发动机发展规划及其性能演变过程进行了梳理,并分析了不同循环类型及循环参数的选择,进行了性能统计分析。然后,介绍了直升机/发动机一体化设计理论的基础与方法。最后本文提出新一代超低排放涡轴发动机的概念,指出降低总耗油量的同时提高功重比,才能实现超低排放。     

提高某铝合金薄壁深孔零件加工质量研究

通过分析某铝合金薄壁深孔零件在加工过程中存在的问题基础上,采用了拉镗拉铰加工内孔,再以轴向定位夹紧的方式加工外形的思路,该方法保证了零件加工精度,解决了该铝合金薄壁深孔零件的加工问题,完全满足生产实际需要,质量稳定可靠,可为类似零件加工提供参考。     

三脉冲冷原子陀螺仪中基于内态演化的拉曼光光强补偿算法

由于在复杂环境中拉曼光功率不稳定会导致原子脉冲的宽度发生改变,从而影响陀螺仪的测量精度.通过对冷原子干涉仪的干涉全过程进行建模,计算得出了陀螺仪在拉曼光改变情形下输出相位的解析表达式,即建立了拉曼光在非近共振条件下强度变化时陀螺仪的输出值与外界载体运动之间的关系.与此同时,基于该解析表达式提出了一种对拉曼光光强的补偿算...     

Halo White Dwarfs and Baryonic Dark Matter

We describe the formation of hot intergalactic gas along with baryonic remnants in galaxy halos. In this scenario, the mass and metallicity of the hot intracluster and intragroup gas relates directly to the production of baryonic remnants during the collapse of galactic halos. We construct a schematic but self-consistent model in which early bursts of star formation lead to a large remnant population in the halo, and to the outflow of stellar ejecta into the halo and ultimately the Local Group. We consider local as well as high redshift constraints on this scenario. This study suggests that the microlensing objects in the Galactic halo may predominantly be 0.5M white dwarfs, assuming that the initial mass function for early star formation favored the formation of intermediate mass stars with m 1M. However, the bulk of the baryonic dark matter in this scenario is associated with the ejecta of the white dwarf progenitors, and resides in the hot intergalactic medium.     

The Primordial Helium-4 Abundance from Observations of a Large Sample of Blue Compact Dwarf Galaxies

We use a sample of 45 low-metallicity H II regions in blue compact dwarf (BCD) galaxies to determine the primordial helium abundance YP with a precision better than 5%. We have carefully investigated the physical effects which may make the He I line intensities deviate from their recombination values such as collisional and fluorescent enhancements, underlying He I stellar absorption and absorption by Galactic interstellar Na I. By extrapolating the Y vs. O/H and Y vs. N/H linear regressions to O/H = N/H = 0, we obtain YP = 0.244±0.002 and 0.245±0.001, respectively, higher than previous determinations (YP = 0.230 - 0.234). Part of the difference comes from the fact that previous investigators have not taken into account underlying He I stellar absorption, especially in the NW component of the BCD I Zw 18 which, because of its extremely low metallicity plays a key role in the determination of YP. We derive a slope dY/dZ = 2.3±1.0, considerably smaller than those derived before. With this smaller slope and taking into account the errors, chemical evolution models with an outflow of well-mixed material can be built for star-forming dwarf galaxies which satisfy all the observational constraints. Our YP gives _bh ₅₀ ² = 0.058±0.007,f consistent with the lower limit set by dynamical measurements and X-ray observations of clusters of galaxies. It is also consistent, within the framework of standard big bang nucleosynthesis theory, with measurements of primordial 7Li in galactic halo stars and with the D/H abundance measured in absorption systems toward quasars by Burles and Tytler (1997).     

自行开发的图形组件在航空发动机设计集成系统中的应用

结合具体开发的图例,阐述了自行开发、应用于航空发动机设计集成系统的图形组件的功能、应用情况和关键技术。