普通高校计算机专业大学生就业问题探析

计算机专业如何迎战IT就业＂寒流＂,提高就业率和就业质量,这是众多高校共同关注的问题。在分析就业形势,认真查找普通高校计算机专业大学生存在问题的基础上,并提出了解决目前IT学生就业的对策和措施。     

数控蒙皮横拉机运动分析与仿真控制

进行了某数控蒙皮横拉机的机构分析,开发了机构运动反解软件.并在UG软件中进行了机构的运动建模与计算机仿真.运动反解与计算机仿真的相互验证,确定运动反解软件的准确性.实现了拉形过程有限元模拟与拉形机作动筒伸缩控制的结合,为该设备的精确控制及效能发挥提供了技术基础.      

椭圆形截面螺旋管道内二次流动的摄动解

从曲线直角坐标系中的Ｎ－Ｓ方程出发,采用摄动方法求解了椭圆形截面螺旋管道内粘性流动。结果表明：一阶挠率项仅影响椭圆形截面上的二次流动,并不影响截面上轴向速度;当轴向压力梯度较小时,二次流动主要受挠率的影响,随着轴向压力梯度的增加,曲率的作用越来越强。     

圆形隧道衬砌与围岩应力的解析法研究

隧道衬砌与围岩的应力分析是隧道设计中一个重要内容。本文基于厦门市东通道海底隧道对圆形隧道衬砌与围岩应力的封闭解析解法进行研究,首先利用MATLAB编制衬砌与围岩应力程序并选用一个已有精确解的实例进行校验,然后对圆形隧道四种工况进行计算并给出相关的衬砌和围岩的分布曲线,最后对计算结果进行了相关分析。     

连接器支架结构优化设计分析

某型连接器支架普遍出现断裂现象,经判断原因是动强度设计不合理,在振动载荷作用下发生疲劳破坏,为了确保支架不出现结构损伤,保证飞行安全,需要进行结构优化设计分析。基于克希霍夫理论,采用有限元分析手段,通过改变厚度、材料与结构形式的方法,对支架进行模态分析与随机响应分析,最终得到了在满足动强度设计要求的情况下质量最轻的支架。根据分析结果总结了一种结构优化设计分析的流程:先改结构形式,用相对系数判断优劣;再选疲劳性能好的材料;最后选择合适的厚度。该流程在本文中得到有效实施,可在今后用于相似结构的优化设计分析。     

热载下三边固支一边简支矩形薄板的解析解

基于薄板的小挠度理论,根据四边简支矩形薄板在横向变温作用下的挠度和内力解答,通过应用虚功原理和叠加原理,推导了三边固支一边简支矩形薄板在横向变温作用下的挠度方程和内力解析解,从而为以后的工程计算提供了理论依据.     

通用加速计算在环幕失真校正中的应用研究

大规模场景的沉浸式投影系统大都以环幕作为显示设备,而由环幕造成的几何失真使系统真实感大大降低。从环幕产生失真的几何原理出发,通过建立投影平面和成像面之间的坐标映射关系,生成了一种几何失真校正的理论模型。同时,研究了一种适于通用加速计算的图形硬件架构CUDA,基于其多线程的硬件执行机制,通过将几何失真的校正矩阵组织成纹理进行多重纹理贴图映射,设计了预失真校正的硬件加速算法,该算法还利用基于权值的超采样技术对加速中的走样进行了设计。最后,对该方法的校正效率和效果进行了实验验证,证明该方法具有更高的场景交互速度和很好的校正效果。     

Analytical expression for distant retrograde orbits around a small natural satellite

An analytical expression for distant retrograde orbits (DROs) is obtained in this study. Owing to the fact that a planar DRO is a closed orbit and can be expressed as an approximately elliptical orbit, respective geometries and periods of DROs are analytically calculated. A switching point, where various properties of planar DROs change abruptly with an increase in the orbital radius, is determined. The Mars–Deimos system is taken as a case study in this work. The proposed method can be applied to cases where the Hill’s approximation of the restricted three-body problem is valid. Numerical calculations are performed to validate the proposed method.     

Observations of the local interstellar medium with the Extreme Ultraviolet Explorer

Because of the strong absorption of extreme ultraviolet radiation by hydrogen and helium, almost every observation with the Extreme Ultraviolet Explorer (EUVE) satellite is affected by the diffuse clouds of neutral gas in the local interstellar medium (LISM). This paper reviews some of the highlights of the EUVE results on the distribution and physical state of the LISM and the implications of these results with respect to the interface of the LISM and the heliosphere. The distribution of sources found with the EUVE all-sky surveys shows an enhancement in absorption toward the galactic center. Individual spectra toward nearby continuum sources provide evidence of a greater ionization of helium than hydrogen in the Local Cloud with an mean ratio of H I/He I of 14.7. The spectral distribution of the EUV stellar radiation field has been measured, which provides a lower limit to local H II and He II densities, but this radiation field alone cannot explain the local helium ionization. A combination of EUVE measurements of H I, He I, and He II columns plus the measurement of the local He I density with interplanetary probes can place constraints on the local values of the H I density outside the heliosphere to lie between 0.15 and 0.34 cm^–3 while the H II density ranges between 0.0 and 0.14 cm^–3. The thermal pressure (P/k = nT) of the Local Cloud is derived to be between 1700 and 2300 cm^–3 K, a factor of 2 to 3 above previous estimates.