止口螺栓连接结构解析建模与阻尼特性分析

针对止口螺栓连接,论文从连接结构轴向拉压力学行为分析出发,提出了可模拟连接非线性刚度和阻尼耗散的扇区模型,基于此进一步构建了弯矩载荷下的非线性解析模型。通过与三维实体有限元模型计算结果的对比分析,验证了所提出模型的有效性,并揭示了连接的非线性刚度特性和迟滞阻尼特性。基于所提出模型研究了关键参数对止口螺栓的阻尼特性的影响规律,结果表明:连接的阻尼耗散能力随弯矩载荷幅值和摩擦因数的增加呈现先增加后降低趋势,而随止口紧度和法兰长度的增加单调增加;法兰长度除对连接的阻尼耗散存在一定影响外,还能显著降低连接结构的等效刚度。      

U型无铁心永磁同步直线电机磁场建模与分析

传统的铁心式直线电机由于铁心开断的影响,造成了横向和纵向边端效应,使推力输出波动较大;无铁心永磁直线电机具有零齿槽效应的优点,结构简单,控制灵活。采用两种解析法求解无铁心永磁同步直线电机气隙磁场的问题,即等效磁势法和等效磁化电流法,同时采用有限元法对电机磁场进行有限元分析,验证解析法磁场解析计算的准确性。最后分析电机主要尺寸对气隙磁场的影响。通过改变电机参数,进行了优化设计,为同类电机的设计与分析提供了参考。     

空气/烟气组合对波转子发动机性能的影响

针对波转子作为燃气轮机高压级构成的波转子发动机,考虑波转子普遍存在的烟气回流、空气排放现象及其形成的空气/烟气工质组合,建立热力学控制方程组,对波转子发动机总体方案进行对比和参数分析,并且基于热力循环模型分析参数影响关系的热力学原理。分析结果表明:烟气回流和空气排放的流量比例的增加会在不同程度上降低波转子发动机的循环功与热效率;烟气回流对总体性能的影响程度小于空气排放;适当提高波转子压比可以在考虑烟气回流和空气排放影响的前提下保持波转子发动机的总体性能。     

基于Matlab/Simulink的航空发动机稳态求解方法研究

基于Matlab/Simulink仿真环境,结合GSP软件提供的通用部件特性,建立了某型大涵道比涡扇发动机的部件级模型.以此模型为基础,建立流量平衡与功率平衡的非线性方程组,并选取高低压转速以及发动机各部件压比为初猜值,对发动机设计点进行稳态求解.对比分析了牛顿-拉夫僧法、拟牛顿法和最速下降法的求解数据,最终选择拟牛顿法作为本发动机模型的稳态求解方法.     

固溶处理时间对2E12铝合金组织和疲劳性能的影响

采用光学金相、扫描电镜、能谱分析以及疲劳寿命测试等方法,研究了495 ℃/1 h和8 h固溶处理对2E12T₄铝合金微观组织和疲劳性能的影响。实验结果表明,延长固溶处理时间可显著减少基体中可溶的Al₂CuMg残留相数量,提高合金元素的过饱和固溶度,因而,自然时效后合金强度相应增加。试样自由表面上的大尺寸残留相在疲劳加载过程中,通过自身断裂或与基体脱粘的两种方式优先诱发疲劳裂纹萌生;并且,这些大尺寸残留相还起到促进疲劳裂纹扩展和连接的作用,导致疲劳辉纹形成时发生开裂形成二次裂纹,因而,延长固溶处理时间减少大尺寸残留相数量可提高2E12铝合金的疲劳寿命。     

The Geology of Mercury: The View Prior to the MESSENGER Mission

Mariner 10 and Earth-based observations have revealed Mercury, the innermost of the terrestrial planetary bodies, to be an exciting laboratory for the study of Solar System geological processes. Mercury is characterized by a lunar-like surface, a global magnetic field, and an interior dominated by an iron core having a radius at least three-quarters of the radius of the planet. The 45% of the surface imaged by Mariner 10 reveals some distinctive differences from the Moon, however, with major contractional fault scarps and huge expanses of moderate-albedo Cayley-like smooth plains of uncertain origin. Our current image coverage of Mercury is comparable to that of telescopic photographs of the Earth’s Moon prior to the launch of Sputnik in 1957. We have no photographic images of one-half of the surface, the resolution of the images we do have is generally poor (∼1 km), and as with many lunar telescopic photographs, much of the available surface of Mercury is distorted by foreshortening due to viewing geometry, or poorly suited for geological analysis and impact-crater counting for age determinations because of high-Sun illumination conditions. Currently available topographic information is also very limited. Nonetheless, Mercury is a geological laboratory that represents (1) a planet where the presence of a huge iron core may be due to impact stripping of the crust and upper mantle, or alternatively, where formation of a huge core may have resulted in a residual mantle and crust of potentially unusual composition and structure; (2) a planet with an internal chemical and mechanical structure that provides new insights into planetary thermal history and the relative roles of conduction and convection in planetary heat loss; (3) a one-tectonic-plate planet where constraints on major interior processes can be deduced from the geology of the global tectonic system; (4) a planet where volcanic resurfacing may not have played a significant role in planetary history and internally generated volcanic resurfacing may have ceased at ∼3.8 Ga; (5) a planet where impact craters can be used to disentangle the fundamental roles of gravity and mean impactor velocity in determining impact crater morphology and morphometry; (6) an environment where global impact crater counts can test fundamental concepts of the distribution of impactor populations in space and time; (7) an extreme environment in which highly radar-reflective polar deposits, much more extensive than those on the Moon, can be better understood; (8) an extreme environment in which the basic processes of space weathering can be further deduced; and (9) a potential end-member in terrestrial planetary body geological evolution in which the relationships of internal and surface evolution can be clearly assessed from both a tectonic and volcanic point of view. In the half-century since the launch of Sputnik, more than 30 spacecraft have been sent to the Moon, yet only now is a second spacecraft en route to Mercury. The MESSENGER mission will address key questions about the geologic evolution of Mercury; the depth and breadth of the MESSENGER data will permit the confident reconstruction of the geological history and thermal evolution of Mercury using new imaging, topography, chemistry, mineralogy, gravity, magnetic, and environmental data.     

基于通用微机的雷达终端系统设计

雷达终端是雷达系统的核心组成部分,有必要采用当前先进的软硬件技术来设计.考虑到雷达终端发展现状,着重分析了雷达的功能要求和系统中的信息流,构建了基于通用微机的模块化、软件化的雷达终端系统,并详细讨论了系统的结构及硬件和软件的设计.系统由通用微机和雷达信号处理板sD754lA来实现,在运行过程中稳定可靠,满足雷达信号数据实时处理和显示的需求.     

一种弹道导弹再入弹道解析方法

在现有再入段解析方法的基础上,考虑更为贴近实际的条件因素,求得一组新的弹道导弹再入弹道解析解.首先,在忽略引力影响的条件下,求解非线性微分方程组,得到零阶速度解和零阶速度倾角;再代入原方程组解出一阶速度、再入段飞行时间、速度倾角及射程的解析表达式;最后通过仿真计算证明了该方法的优越性.     

超音速气流中横向喷射氢气流场数值模拟

本文通过应用Mac Cormack显式时间分裂法和Baldwin-Lomax修正的代数湍流模型求解二维可压缩的N-S方程和混气组分方程,对超音速气流中横向喷入氢气后的流场进行了数值模拟。计算结果示出了流场中速度矢量分布,静压、静温和氢气质量分数的等值线分布,反映出了喷嘴附近流场回流区的大小及可能的点火位置,从而为超燃冲压发动机的设计工作提供理论指导。     

多钉连接件钉传载荷计算的一个解析方法

对多钉连接件钉传载荷的计算问题提出了一个解析分析方法,推导了求解钉载的线性代数方程组并给出了若干算例。该方法使用方便,并具有工程分析所要求的精度。