试论我国财务软件服务体系的建立

我国财务软件发展至今,总体上看还很不健全,针对实践中遇到的问题,对财务软件服务体系的建立做一些实证性上的探讨。     

2.5D石英纤维织物增强二氧化硅基复合材料弯曲性能测试研究

简要介绍了2．5D石英纤维织物增强二氧化硅基复合材料弯曲性能测试装置，通过对比试验研究了试样跨厚比、变形测量等对材料弯曲性能的影响，用数理统计的方法对总体均值进行了显著性检验，合理确定了材料弯曲性能测试的试验参数。     

TC6钛合金棒材热处理工艺研究

对TC6钛合金φ20mm～φ120mm不同规格棒材进行了普通退火、双重退火、等温退火、固溶时效等热处理方法和热处理制度研究,并对比分析了热处理制度和组织、性能之间的影响关系,结果表明,TC6钛合金的组织和性能对热处理工艺敏感,应根据半成品规格、类型、截面形状、使用温度、受力情况以及设备条件等诸多因素选择合适的热处理方法和制度,才能达到强度、塑性和韧性的最佳匹配。研究结果证实普通退火是一种简单易行的退火制度,适用于飞机结构用中等规格棒材等半成品的退火,进一步提出了TC6钛合金棒材的热处理工艺选择原则。     

一种计算再生冷却推力室温度场的方法

为了能够快速而准确地得到再生冷却推力室的温度分布,建立了一种计算再生冷却推力室温度场的方法。首先建立了轴对称推力室的一维冷却模型,并使用换热经验公式,得到了推力室壁面在轴线方向上的温度分布;其次建立了推力室的冷却套二维导热模型,使用数值模拟的方法和一维计算的结果,得到了冷却套的温度场。然后使用这种方法研究了气壁材料、气壁厚度和冷却液流量对推力室再生冷却的影响,获得了比较满意的结果。从计算时间和准确性来说,这种方法能够为推力室的优化设计和性能估算提供参考。      

某型航改燃机振动特性研究

介绍了某型航改燃机整机振动设计特性及其现场调试并作出试验总结     

基于CCD的底片判读仪透射屏厚度精确测量

提出了一种利用线阵CCD传感器作为接收装置，以8253编程芯片实现自动测量并实时显示测量结果的底片判读仪透射屏厚度测量系统。文中主要论述了该系统的工作原理和软硬件的实现途径，并分析了系统的测量误差；文章最后列出了实测数据，证明了系统的可行性和先进性。     

ARALL层压板结构疲劳性能分析

目前在航空领域发展非常迅速的ARALL层压板结构和芳纶预浸料的制造工艺,预浸料在具有高的抗疲劳特性和拉伸特性的ARALL层压板结构中起到非常重要的承力和抗疲劳作用。本结构所采用的制造方法是纤维拉伸法,是一种能使ARALL结构的铝板层具有残余压应力,使纤维层具有残余拉应力的方法,从而改善了材料本体的抗疲劳性能。     

变几何喉道对超燃冲压发动机点火与燃烧性能的影响

1引言超燃冲压发动机能高速飞行且能利用空气中的氧气作氧化剂,增加了有效载荷,因而备受重视,但它需要在较高的飞行马赫数下才能工作,因此受到较大的限制。由于双模态超燃冲压发动机可以将工作飞行马赫数下限降低至Ma=3,发动机在飞行马赫数Ma=3~6时以亚燃冲压模态工作,在马赫数     

教师在大学生学风养成方面的影响与作用

面对当前高等教育从“精英教育”走向“大众教育”，高校面临许多新的现象和问题。学风问题是每一时期，每一层次的教育都存在的问题，针对当前高职高专学生的学风养成中教师所应发挥的作用，进行了调研和分析，以期对形成良好的学风有所裨益。     

2001 Mars Odyssey Mission Summary

The 2001 Mars Odyssey spacecraft, now in orbit at Mars, will observe the Martian surface at infrared and visible wavelengths to determine surface mineralogy and morphology, acquire global gamma ray and neutron observations for a full Martian year, and study the Mars radiation environment from orbit. The science objectives of this mission are to: (1) globally map the elemental composition of the surface, (2) determine the abundance of hydrogen in the shallow subsurface, (3) acquire high spatial and spectral resolution images of the surface mineralogy, (4) provide information on the morphology of the surface, and (5) characterize the Martian near-space radiation environment as related to radiation-induced risk to human explorers. To accomplish these objectives, the 2001 Mars Odyssey science payload includes a Gamma Ray Spectrometer (GRS), a multi-spectral Thermal Emission Imaging System (THEMIS), and a radiation detector, the Martian Radiation Environment Experiment (MARIE). THEMIS and MARIE are mounted on the spacecraft with THEMIS pointed at nadir. GRS is a suite of three instruments: a Gamma Subsystem (GSS), a Neutron Spectrometer (NS) and a High-Energy Neutron Detector (HEND). The HEND and NS instruments are mounted on the spacecraft body while the GSS is on a 6-m boom. Some science data were collected during the cruise and aerobraking phases of the mission before the prime mission started. THEMIS acquired infrared and visible images of the Earth-Moon system and of the southern hemisphere of Mars. MARIE monitored the radiation environment during cruise. The GRS collected calibration data during cruise and aerobraking. Early GRS observations in Mars orbit indicated a hydrogen-rich layer in the upper meter of the subsurface in the Southern Hemisphere. Also, atmospheric densities, scale heights, temperatures, and pressures were observed by spacecraft accelerometers during aerobraking as the spacecraft skimmed the upper portions of the Martian atmosphere. This provided the first in-situ evidence of winter polar warming in the Mars upper atmosphere. The prime mission for 2001 Mars Odyssey began in February 2002 and will continue until August 2004. During this prime mission, the 2001 Mars Odyssey spacecraft will also provide radio relays for the National Aeronautics and Space Administration (NASA) and European landers in early 2004. Science data from 2001 Mars Odyssey instruments will be provided to the science community via NASA’s Planetary Data System (PDS). The first PDS release of Odyssey data was in October 2002; subsequent releases occur every 3 months.