Soho Observations of Density Fluctuations in Coronal Holes

In recent UVCS/SOHO White Light Channel (WLC) observations we found quasi-periodic variations in the polarized brightness (pB) in the polar coronal holes at heliocentric distances of 1.9 to 2.45 solar radii. The motivation for the observation is the 2.5D MHD model of solar wind acceleration by nonlinear waves, that predicts compressive fluctuations in coronal holes. In February 1998 we performed new observations using the UVCS/WLC in the coronal hole and obtained additional data. The new data corroborate our earlier findings with higher statistical significance. The new longer observations show that the power spectrum peaks in the 10–12 minute range. These timescales agree with EIT observations of brightness fluctuations in polar plumes. We performed preliminary LASCO/C2 observations in an effort to further establish the coronal origin of the fluctuations. This revised version was published online in June 2006 with corrections to the Cover Date.     

Analysis of Performance Degradation in CdS Solar Cells

The effect of changes in five physically meaningful parameters on the I-V (current-voltage) curve of a CdS solar cell is calculated. Comparisons between the calculated data and performance data obtained from degraded solar cells are made. The parameter that changed to cause the degradation in each cell becomes apparent.     

7. Dynamics,winds, circulation and turbulence in the atmosphere of venus

With the possible exception of the lowest one or two scale heights, the dominant mode of circulation of Venus' atmosphere is a rapid, zonal, retrograde motion. Global albedo variations in the ultraviolet may reflect planetary scale waves propagating relative to the zonal winds. Other special phenomena such as cellular convection in the subsolar region and internal gravity waves generated in the interaction of the zonal circulation with the subsolar disturbance may also be revealed in ultraviolet imagery of the atmosphere. We discuss the contributions of experiments on the Orbiter and Entry Probes of Pioneer Venus toward unravelling the mystery of the planet's global circulation and the role played by waves, instabilities and convection therein.     

Initial observations of low energy charged particles near the Earth's bow shock on ISEE-1

We report initial measurements from the ULECA sensor of the Max-Planck-Institut/University of Maryland experiment on ISEE-1. ULECA is an electrostatic deflection — total energy sensor consisting of a collimator, deflection analyzer and an array of solid state detectors. The position of a given detector, which determines the energy per charge of an incident particle, together with the measured energy determine the particle's charge state. We find that a rich variety of phenomena are operative in the transthermal energy regime (10 keV/Q to 100 keV/Q) covered by ULECA. Specifically, we present observations of locally accelerated protons, alpha particles, and heavier ions in the magnetosheath and upstream of the Earth's bow shock. Preliminary analysis indicates that the behavior of these locally accelerated particles is most similar at the same energy per charge.     

面向制造业的逆向供应链中的产品回收

针对制造业中产品回收的问题,在分析逆向供应链特点的基础上,讨论了逆向供应链中的产品回收过程、产品回收网络和产品回收的难点,为进一步定量分析产品回收网络奠定了基础.     

基于多Agent卫星遥测数据实时监测与诊断技术

为了提高根据遥测数据进行卫星故障诊断的速度与精度,提出了集成多信号模型诊断Agent、模糊诊断Agent以及专家系统诊断Agent等多Agent监测与诊断系统。多信号模型诊断Agent,采用模糊阈值进行监测,并引入可信度因子对Deb原实时诊断推理方法做了改进,解决了Deb方法可能因虚警而导致的诊断结果冲突的问题。模糊诊断Agent采用Mamdani算法,能给出部件故障的可能性。专家系统诊断Agent采用基于规则的产生式系统,同时采用加权不确定推理解决了规则的不确定性问题。研究了3种诊断Agent的协作方式,采用D-S证据理论对各Agent的诊断结果进行决策融合,给出故障元件的置信区间。通过某卫星仿真遥测数据验证,该集成诊断系统充分利用了各种诊断方法的优点,诊断精度高且速度快(一般诊断时间小于0.3秒,PIII800/256M计算机),适用于卫星地面站对卫星遥测数据进行自动实时在线监测与诊断推理。     

多重网格技术在复杂粘性流场计算中的应用及研究

流体力学控制方程的数值求解过程中,当网格加密、粘性效应强或来流马赫数低的时候,流场收敛非常缓慢。本文在多块网格、LUSGS隐式格式基础上采用多重网格技术,计算了NLR7301case#1两段翼型的低速绕流及DLRF4跨声速流场,在复杂二维、三维粘性流场求解中获得了满意的加速收敛效果。文中还比较了V循环、W循环的加速效率,为多重网格的工程应用奠下基础。     

激波风洞重模型气动力试验研究

在激波风洞上进行气动力试验时,风洞启动时巨大的冲击载荷使模型-天平受到充分的激励,从而形成惯性干扰力,并与真实气动力混杂在一起,甚至完全覆盖气动力,降低了试验精准度,使得试验模型的质量受到极大的限制。本文介绍了CARDC-dia.2米激波风洞进行大、重模型的压电天平气动力试验研究情况,包括天平设计、天平校准、惯性补偿和风洞试验等几个方面。研究结果表明:气动力试验模型质量可从过去的500g增加到8kg,模型长度可达1m。从而提高了激波风洞测力试验能力,能满足高超声速飞行器试验的需求。     

900℃动态应变计的研制与应用

为了对某型航空发动机涡轮转子叶片在900℃高温下进行动应力测试,研制了900℃动态应变计。分别从研制方案、材料的选取、应变计的制作、焊点的焊接形式与疲劳寿命和应用测试等方面进行了详细的阐述和分析。该成果成功地应用于某型发动机台架涡轮转子叶片的动应力测试中。     

Track-before-detect procedures for early detection of moving target from airborne radars

In this paper we present a family of track-before-detect (TBD) procedures for early detection of moving targets from airborne radars. Upon a sectorization of the coverage area, the received echoes are jointly processed in the azimuth-range-Doppler domain and in the time domain through a Viterbi-like algorithm that exploits the physically admissible target transitions between successive illuminations, in order to collect all of the energy back-scattered during the time on target (TOT). A reduced-complexity implementation is derived assuming, at the design stage, that the target does not change resolution cell during the TOT in each scan. The constant false alarm rate (CFAR) constraint is also englobed in the proposed procedures as well as the possibility of working with quantized data. Simulation results show that the proposed algorithms have good detection and tracking capabilities even for high target velocities and low quantization rates.