液体火箭POGO振动时域分析方法研究

建立了液体火箭的动力学方程,将其化为具有初值问题的微分方程进行求解,以实现POGO振动特性的时域仿真,在微分方程的数值求解的基础上,获得液体火箭POGO振动的动态响应特性。根据液体火箭POGO振动主要参数,如结构特征点处的加速度,泵入口处的压力脉动等的时间历程的收敛或发散情况及飞行特征秒,来判断POGO振动是否发生或发生的时间。     

基于最近服务的层次式网格信任模型

阐述了网格环境中信任模型的需求,并分析了传统网格信任模型的优缺点,由此提出了基于最近服务的层次式网格信任模型,设计了相应的计算公式.与传统的信任模型相比较,该模型占用网格资源少、信任评估复杂度低、可伸缩性强,能够较好地抑制网格环境下的恶意评价和协同作弊的威胁.采用改进后的网格仿真工具GridSim进行模拟实验,结果表明该信任模型提高了网格系统的可靠程度.     

奈达功能对等视角下英语广告中仿拟的翻译策略

本文运用尤金·奈达的功能对等理论分析了仿拟在英语广告中的应用与翻译方法,英语广告的翻译应以汉语受众的接受心理为基础,追求功能对等的翻译效果,为产品赢得更大的效益.     

带宽弦叶片的盘片耦合振动特性研究

为确定盘片系统将发生的耦合共振,建立了带宽弦叶片的盘片耦合系统的基本重复扇区的有限元模型,并采用波传播技术对耦合系统进行了振动特性的计算分析.指出了宽弦叶片在振动中表现出的特有振型,以及随转速的变化规律.分析了盘片耦合后的振动特性,以及叶片各阶振动频率随节径数变化的规律.      

面向用户的以太网可用性模型

带冲突检测的载波侦听多路访问协议(CSMA/CD)可以有效的解决竞争,提供高的吞吐量和低的延迟时间,并且成为了局域网设计中颇具吸引力的协议.基于计算机以太网CSMA/CD协议,面向用户探讨以太网可用度模型.通过定义工作站"拥塞状态"和"空闲状态",建立基于网络带宽、时隙的可用度模型.以信息成功发送概率作为衡量以太网可用性的指标.根据以太网中工作站的数量、平均字节长度、单机产生数据的速率以及单机数据重传速率对可用性影响的分析表明,随着局域网中接入的工作站的数量的增加在相同的时间内局域网的可用度将降低.随着数据产生率的升高,局域网的可用度将首先升高,当网络达到饱和后再增加数据产生率,局域网的可用度将降低.提高数据的重传率能够提高局域网的可用度.根据以上的分析,通过合理的设置网络参数,可以使局域网达到理想的可用度.      

复合材料转动壳体动力特性分析

根据转动壳体的动力学方程,在利用DMAP对大型有限元软件MSC/NASTRAN二次开发的基础上,采用有限元方法对复合材料层合壳体转动状态下的动力特性进行了研究,分析了科氏力、离心力和横向剪力对固有频率的影响,并与实验结果进行了比较.结果显示由于科氏力的作用,即使在动坐标系下,层合壳体也会出现频率不等的前后行波,横向剪力使壳体的固有频率降低,且随着壳体厚径比的增加其影响显著增加.      

带QoP反馈的实时视频服务质量控制框架

分析了实时视频在现有"尽力而为"IP网络上传输所面临的带宽、延迟和丢失等问题,介绍了需要采用的拥塞控制和差错控制等应用级服务质量控制策略,并提出了一种联合的支持应用级服务质量控制的实时视频传输框架.该框架既考虑了网络资源的动态变化和影响,又兼顾了视频的服务质量调整对视频的表现质量的限制因素,充分利用了服务质量和表现质量之间的映射关系,具有更广泛的实用价值.      

空间等离子体导致高电压太阳阵的电流收集

给出一种能方便计算空间等离子体引起高电压太阳阵（HVSA）电流收集的理论统计模式，通过对物理过程分析认为空间等离子体致HVSA的功率损耗对HVASA的设计是不应忽视的。     

Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

WAKE GEOMETRY CALCULATIONS FOR TILT-ROTOR USING VISCOUS VORTEX METHOD

A tilt-rotor unsteady flow analytical method has been developed based upon viscous vortex-particle meth- od. In this method, the vorticity field is divided into small assembled vortex particles. Vortex motion and diffusion are obtained by solving the velocity-vorticity-formed incompressible Navier-Stokes equations using a grid-free La- grangian simulation method. Generation of the newly vortex particles is calculated by using the Weissinger-L lifting surface model. Furthermore, in order to significantly improve computational efficiency, a fast multiple method （FMM） is introduced into the calculation of induced velocity and its gradient. Finally, the joint vertical experimen- tal （JVX） tilt-rotor is taken as numerical examples to analyze. The wake geometry and downwash are investigated for both hover and airplane modes. The proposed method for tilt-rotor flow analysis is verified by comparing its re- sults with those available measured data. Comparison indicates that the current method can accurately capture the complicated tilt-rotor wake variation and be suitable for aerodynamic interaction simulation in complex environ- ments. Additionally, the aerodynamic interactional characteristics of dual-rotor wake are discussed in different ro- tor distance. Results show that there are significant differences on interactional characteristics between hover mode and airplane mode.