带副翼三维机翼绕流的N-S方程解

提出了一种求解带副翼偏转三维机翼绕流的N-S方程计算方法。采用对接分区网格与分区求解算法的结合,有效地求解绕此外形的复杂流动。提出了一种满足通量守恒的内边界耦合条件。数值方法中选用vanLeer分裂格式离散无粘通量项,并构造了一种Limiter函数以保证TVD性质,采用中心差分格式来离散粘性通量项。数值算例表明该方法是求解带操纵面偏转的机翼绕流的有效方法。     

带副翼三维机翼绕流的Euler方程解

提出了一种求解带副翼偏转三维机翼绕的Ｅｕｌｅｒ方程计算方法。采用对接分区网格民分区求解算法的结合,有铲地求解绕引外形的复杂流动,提出了一种满足通量守恒的内边界耦吉选用ＶａｎＬｅｅｒ分裂格式离散玩粘通量项,并构造了一种Ｌｉｍｉｔｅｒ函数以保证ＴＶＤ性质。数值算例表明本方法是求解带操纵纵面偏转的机翼绕流的有效方法。     

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.     

BIT和ATE组合测试技术及其应用

详细介绍了BIT和ATE组合测试技术及其在机载电子设备测试与故障诊断的具体应用。应用表明BIT和ATE组合测试技术可有效提高设备的测试性。     

某型机外形数模修形设计

在某型机外形数模修形设计过程中,探讨如何确定修形原则,即针对存在各种问题的曲面形态,如何确定不同的修形方法,使整个飞机外型数模达到光顺性、结构可实施性、曲面连续性要求。