磁场影响葡萄糖氧化酶活性的研究

以尼龙网作载体，用戊二醛交联将区区糖氧化酶（ＧＯＤ）固定装成酶柱并联结于流动体系中，采用流动注射分光光度法研究磁场对固定化ＧＯＤ催化活性的影响。结果表明，在０℃、５℃、４５℃下以１．０×１０＾－２ｍｏｌ．Ｌ＾－１的葡萄糖为底物及５５℃下以０．１ｍｏｌ＾－１的葡萄糖为底物时，０．２２Ｔ静有显著提高固定化ＧＯＤ的反应速度，且磁场效应与底物浓度及磁场作用时间有关。用动力学方法考察了不同强度的磁场对溶解Ｇ     

压力探针临壁效应的试验与计算

临壁效应会使压力探针的测量结果发生误差。由于探针属非流线形物休，所以其临壁效应的机理与流线形的机翼不同，不能简单套用机翼的结论．对圆柱三孔针的试验结果表明，可以用叠加点涡的方法来描述其临壁效应。点涡强度随离壁距离的减少而增强．     

多媒体教学中视觉效果的设计

本文根据人眼的视觉特性,分析了多媒体教学中视觉效果的影响因素,讨论了多媒体教学中视觉效果的设计方法,指出对多媒体教学视觉效果影响较大的是相邻线条的时距、亮度、色彩、背景和视矩,并给出了相邻线条的最小间距,最小观察距离,观察方向和观察距离的计算公式。     

疏透型防护林绕林流场的PIV实验研究

利用粒子图像测速仪(PIV),采用2帧 互相关的分析方法,对疏透型防护林流场的流动特征在风洞中进行实验研究,获得绕林流场的速度矢量图、速度等势线图和涡量场图。实验中选用的防护林疏透度分别为0%,30%,40%,60%。在各种疏透度下的防护林中,疏透度为0%的防护林近尾流区平均沿流速度衰减幅度大,但恢复也快,且有最高的平均垂直速度。疏透度为30%和40%的防护林绕林流场非常相似,其中疏透度为30%的林带,林后平均沿流速度恢复较慢,且气流扰动较小,具有良好的防风固沙作用。     

Blockage effect on the flow around a cylinder probe in calibration

Flow around a 2-D cylinder pressure probe placed in uniform flow,free jet flow,and wind tunnel flow was analyzed with potential flow theory and simulated with numerical method.Blockage effect was investigated under several typical flow Mach numbers.The result from numerical simulation shows a similar trend to the one from potential flow method while varies in quantity.Wind tunnel walls accelerate the flow near the probe and thus produce a blockage effect;Boundary of free jet flow,however,decelerates the flow and thus produces a "negative" blockage effect.A maximum incoming Mach number exists when the probe is calibrated in wind tunnel in high subsonic condition due to choking caused by shocks and shock induced separation.The critical Mach number varies with blockage ratio,which makes high Mach number impossible to achieve in large blockage ratio condition.The blockage effect itself is unavoidable for calibration or measurement although a sufficiently small blockage ratio brings minor effect.Correction can be implemented based on the numerical simulation result presented in this paper and further works.      

海浪作用下舰载武器IMU输出建模与仿真实现

在海浪作用下舰船载体运动方程极为复杂,文章在对运动方程不作任何简化的情况下,给出了方程的数值解,并在此基础上,考虑杆臂效应的存在,给出了舰载武器的IMU输出模型的仿真实现。研究表明,利用此精确模型能够直接对舰载武器IMU的性能作出有效评估,从而大大减少测评周期和成本。     

An improved prediction model for corner stall in axial compressors with dihedral effect

Corner stall predictions are important and difficult in axial compressors. However, all of the prediction models have proved to be ineffective for advanced compressor blades, which tend to use the combined sweep and dihedral. As for the prediction parameter DL, although it effectively modeled the effects of the adverse pressure gradient and secondary flow, it failed to predict the corner stall of curved blades because the model failed to consider the intersection of the boundary layer at the corner region. In this paper, the shape factor gradient Ψ of the boundary layer at the corner region was investigated by numerically studying specially shaped expansion pipes under different adverse pressure gradients. The improved prediction parameter DJ was presented based on the model of Ψ and the circumferential pressure gradient ξ. A comparison of the critical range of the prediction parameters DL and DJ was investigated using the NACA65 cascade database, which was established by a numerical method. Then, the stall criterion was validated according to the experimental results of various test facilities with different blade geometries and experimental conditions. The results show that the improved prediction parameter is able to predict the corner separation/stall flows and is in good agreement with the experimental results for axial compressors with three-dimensional designed blades.     

Experimental of combustion instability in NTO/MMH impinging combustion chambers

This paper presents an experimental study into dynamics of chamber pressure and heat release rate during self-excited spinning and standing azimuthal mode in NTO/MMH (nitrogen tetroxide/monomethylhydrazine) impinging combustion chambers. Nine cases including two combustion chamber configurations were conducted. The operating conditions of all unstable cases were located in the instability region according to Hewitt empirical correlation. The results show that chamber pressure oscillations keep pace with the corresponding OH* chemiluminescence intensity over the whole combustion region in the spinning and standing modes. It is indicated that the Rayleigh index is positive over the whole combustion area in all the unstable cases. A significant supersonic flame front structure of the first-order spinning mode was found in a cylindrical chamber, which means that a detonation wave could exist in the cylindrical chamber without a center body. The pressure and heat release rate oscillations at the pressure node are nonnegligible although their amplitudes are lower than those at the pressure antinode in the first-order standing mode with an annular chamber. Besides, the dominant frequency of pressure and heat release rate oscillations at the pressure node is twice as high as that at the pressure antinode.     

Aero-optical effects simulation technique for starlight transmission in boundary layer under high-speed conditions

Aero-optical effects for starlight transmission in the high-speed flow field will reduce the accuracy of the star sensor on an aircraft. Numerical simulations for aero-optical effects usually require plenty of calculations, which cause difficulties when designing a celestial navigation system for a high-speed aircraft. In this study, an Aero-Optical Simulator For Starlight Transmission (AOSST) in the boundary layer is developed. It effectively reduces the computational burden compared to that of the widely used CFD simulation, and it achieves satisfactory accuracy. In this simulator, gas ellipsoids satisfying certain design rules are used to simulate coherent density structures in boundary layers. Design rules for the gas ellipsoids are found from published experimental and high-fidelity CFD simulation results. The generated wavefront distortion by AOSST is anchored with the scale law for aero-optical distortion in the boundary layer by determining some control parameters, which enables the simulator to output reliable results over a wide range of flight states. Four numerical examples are provided to verify the performance of AOSST. The results demonstrate that AOSST is able to simulate the directional dependence of aero-optical distortions in boundary layers, the variation trend of distorted wavefront shapes with Reynolds number, and the grayscale distribution on the disturbed star map.     

Calibration errors in determining slant Total Electron Content (TEC) from multi-GNSS data

The global navigation satellite system (GNSS) is presently a powerful tool for sensing the Earth's ionosphere. For this purpose, the ionospheric measurements (IMs), which are by definition slant total electron content biased by satellite and receiver differential code biases (DCBs), need to be first extracted from GNSS data and then used as inputs for further ionospheric representations such as tomography. By using the customary phase-to-code leveling procedure, this research comparatively evaluates the calibration errors on experimental IMs obtained from three GNSS, namely the US Global Positioning System (GPS), the Chinese BeiDou Navigation Satellite System (BDS), and the European Galileo. On the basis of ten days of dual-frequency, triple-GNSS observations collected from eight co-located ground receivers that independently form short-baselines and zero-baselines, the IMs are determined for each receiver for all tracked satellites and then for each satellite differenced for each baseline to evaluate their calibration errors. As first derived from the short-baseline analysis, the effects of calibration errors on IMs range, in total electron content units, from 1.58 to 2.16, 0.70 to 1.87, and 1.13 to 1.56 for GPS, Galileo, and BDS, respectively. Additionally, for short-baseline experiment, it is shown that the code multipath effect accounts for their main budget. Sidereal periodicity is found in single-differenced (SD) IMs for GPS and BDS geostationary satellites, and the correlation of SD IMs over two consecutive days achieves the maximum value when the time tag is around 4?min. Moreover, as byproducts of zero-baseline analysis, daily between-receiver DCBs for GPS are subject to more significant intra-day variations than those for BDS and Galileo.