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.     

海上小井眼脉冲空化射流发生器射流特性室内试验研究

为了经济地开发海上边际油气资源,将小井眼单通道井井身结构及水力脉冲空化射流提速技术相结合研制出了小尺寸(外径为120mm)水力脉冲空化射流发生器,并采用室内试验研究了其射流特性。分析了其在不同排量下的出口压力脉动频率、入出口压力脉动振幅、工具压耗等参数和自激振荡喷嘴的射流特性。研究表明,出口压力脉动频率与排量呈线性增大关系,入口及出口压力脉动振幅随排量增大而呈增大趋势,工具压耗与排量呈2次增大关系,自激振荡喷嘴能够产生负压和空化效应。     

70kN载荷应变天平校准系统研制进展

研制了70kN量级的应变天平校准系统,以满足2m量级高速风洞测力试验天平的静态校准需求。70kN载荷应变天平校准系统基于传统的单元校准方法,采用四自由度复位式体轴系自动校准方案,加载力源为标准砝码,采用砝码独立控制技术的自动加载装置实现天平校准载荷的自动加载。砝码产生的重力通过双十字铰链施力定位装置和刚性加载头准确地传递到天平上,无间隙复位传动机构可以保证天平的精确复位。建成后的校准系统可满足20～70kN量程范围的杆式天平和环式天平等不同类型天平的校准需求。     

全内反射测速技术(TIRV)中界面隐失波基准光强I0的确定

基于隐失波全内反射的测速技术TIRV (Total internal reflection velocimetry)是微纳流动中测量壁面附近几百纳米范围内速度的有效方法。隐失波的光强分布I (z)随离开壁面的高度z指数衰减。若荧光粒子位于光强分布中,其亮度也将符合此指数关系,通过测量粒子亮度可确定粒子的垂向位置z,而确定隐失波的基准光强I0是该技术的关键之一。基于粒子近壁Boltzmann浓度分布、粒子粒径不均匀性和隐失波光强公式,给出了粒子亮度概率密度分布的数值解。实验测量粒子统计亮度分布后,依据实验和理论分布相同原则可定量确定基准光强I0。采用φ100nm和φ250nm 荧光粒子验证此方法并定量分析了粒径分散性对确定 I0的影响。进一步采用φ100nm粒子进行近壁速度测量实验,结果验证了本方法的有效性。