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。     

细长体出水动力学的实验研究及数值模拟

航行体出水过程涉及到气液两相交界,流场是非定常且高度非线性的,是一个非常复杂的过程。为了深入研究该问题,采用实验和数值模拟相结合的方法研究了细长体垂直出水过程的水动力特性。实验在二维水箱中进行,采用高速摄影仪拍摄了不同速度下细长体垂直出水流场。数值模拟采用 VOF 模型,结合动网格和 UDF 技术对相应的实验工况进行了模拟。研究了细长体水下运动过程中空泡的生长和溃灭机理,以及细长体出水时对自由液面的干扰规律。实验研究表明:(1)细长体在完全出水时刻出水速度发生突增;(2)随着细长体速度的增大,空泡产生的部位是从尾部开始,然后再在头部出现;(3)当细长体头部没有局部空泡产生的时候,细长体出水时会造成明显液面隆起现象,当细长体头部产生局部空泡后,细长体出水时,没有明显液面隆起现象,但是会产生“喷溅”现象。数值计算表明:在不产生空泡的情况下,细长体头部接近水面到完全出水的过程中,自由液面都会隆起,尾部出水时液面隆起的程度比头部出水时大。通过比较数值计算结果与实验结果,两者吻合较好。     

高分辨率星载SAR总体参数分析

本文详细分析了高分辨率星载ＳＡＲ的方位分辨率、距离徒动效应以及影响脉冲重复频率选择的因素。同时论述了分辨率、测绘带宽，模糊度、脉冲重复频率之间的相互制约关系。并给出了计算机仿真结果。     

高温超导X波段带通滤波器研制

本文选用 10× 15× 0 .4 4 m m3双抛 L a Al O3衬底上外延生长的优质双面钇系高温超导 (HTSC)薄膜的Yba2 Cu3O7(YBCO) ,设计并制作了结构紧凑的高温超导发夹线微波窄带滤波器。该滤波器工作温度在 90 K以下 ,77K时指标为 :中心频率 9.4 8GHz,3d B相对带宽 1.1% ,带内最小插损 0 .36 d B,带外抑制大于 4 5 d B。另外 ,本文还介绍了高温超导滤波器的精确设计方法 ,并对高温超导滤波器的功率容载、制作等问题进行了讨论 ,同时还研制了具有实用意义的全密封高温超导滤波器外壳 ,仅需液氮制冷即可进入工作状态 ,输入、输出采用 SMA密封接头。