时空守恒元和解元方法的爆震波一维数值模拟

运用基元化学反应模型和流体力学的基本原理，建立了脉冲爆震发动机一维非定常反应流数学模型。应用一种改进的时空守恒元和解元(CESE)方法建立控制方程的差分格式，针对化学反应源项的刚性问题，在对非线性源项进行线性化处理的基础上，应用隐式梯形方法实现源项的积分。对氢氧爆震波的形成和传播过程进行数值计算，结果表明，应用CESE方法和基元化学反应模型能够成功地模拟氢氧爆震波的精细结构。     

飞机风挡鸟撞动响应分析方法研究

建立了鸟体模型和风挡玻璃破坏准则,形成了一套完整的风挡鸟撞动响应分析方法。并对某型号风挡进行了鸟撞动响应分析,得出了鸟的运动轨迹和风挡的位移、应力、应变响应以及风挡玻璃的鸟撞临界速度,经与试验结果比较,两者吻合较好。     

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。     

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.     

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.     

ATE综合校准系统的软件设计及实现

通用自动测试设备（ATE）的测量准确性、可靠性会直接影响飞机综合保障的质量,因此,对此检测设备进行全面有效的测试校准,是确保测试系统完成任务的关键。为了保障测试数据准确可靠和量值传递统一及实现现场的系统性校准工作,本课题以通用自动测试设备为对象,建立了一套基于虚拟仪器技术基础上的综合校准系统。本文对系统的软件结构设计进行了分析和设计,以LCOD原型生命周期为基础,使用了面对组件的设计模式,设计和实现了软件功能,使得该系统具有一定的兼容性和可移植性,并且为扩展留下了接口,同时保证了校准数据的可靠性和精确性。     

电脉冲除冰(EIDI)系统电动力学模型分析

总结了电脉冲除冰(EIDI)系统电动力学模型的研究现状,针对几种常见的计算模型进行了分析,以Bernhart-Schrag模型为例,重点阐述了电动力学模型的理论基础、等效模型的建立以及状态方程的求解,分析了模型的正确性.针对由环状平绕线圈及金属平板构成的EIDI简化系统,Bernhart-Schrag模型可以预测通电线...     

八节点Hamiltonian等参元列式

为了使平面八节点等参元的优越性在弹性力学Hamilton正则方程的半解析法得到应用。结合弹性材料修正后的Hellinger—Reissner（H—R）变分原理和二次插值函数表达平面外应力和位移函数,建立了Hamilton正则方程的八节点等参元列式。首先简要地介绍了弹性材料修正后的H—R变分原理．然后用二次插值函数表示平面外应力和位移变量,并详细地推导了Hamilton正则方程的八节点等参元列式。数值实例结果证明了本文等参元列式的正确性。     

含弱粘结界面复合材料层合板的半解析法

采用线性弹簧模型表征界面弱粘结特性．并运用了Hamilton正则方程的半解析方法处理界面弱粘结对复合材料层合板弯曲问题的影响。首先简要地介绍了弹性材料修正后的H—R变分原理和Hamilton元,然后着重推导了弱粘结界面的线弹簧模型的平面元素列式及正则方程的半解析法的控制方程。最后根据界面传递关系建立了弱粘结层合板的控制方程。数值实例结果证明了本文方法的正确性。