基于气隙磁场定向的无轴承异步电机非线性解耦控制

无轴承异步电机是一个强耦合的非线性复杂系统，实现了其电磁转矩和径向悬浮力之间的解耦控制是该电机稳定运行的前提。本在研究电机磁悬浮机理的基础上，提出了利用气隙磁场定向控制来实现两之间的动态解耦控制。仿真实验也证明该控制算法不仅能实现电机稳定的悬浮，而且使电机具有良好的调速性能。     

NEW APPROACHES OF MUSCL SCHEMES FOR COMPRESSIBLE FLUIDS

The MUSCL scheme for compressible gas dynamicsis studied in this paper. We propose a new type of Euleri-an MUSCL scheme, which evaluates the intercell flux athalf time step. The intercell flux is comptuted from char-acteristic equations with the data which traced backthrough the approximatecharacteristic from the edge athalf time step. The data is classified in several differenttypes, depending on the characteristic directions of data.We also present a general procedure of oscillation-fre…     

Dust Environment Modelling of Comet 67P/Churyumov-Gerasimenko

Dust is an important constituent of cometary emission; its analysis is one of the major objectives of ESA’s Rosetta mission to comet 67P/Churyumov-Gerasimenko (C–G). Several instruments aboard Rosetta are dedicated to studying various aspects of dust in the cometary coma, all of which require a certain level of exposure to dust to achieve their goals. At the same time, impacts of dust particles can constitute a hazard to the spacecraft. To conciliate the demands of dust collection instruments and spacecraft safety, it is desirable to assess the dust environment in the coma even before the arrival of Rosetta. We describe the present status of modelling the dust coma of 67P/C–G and predict the speed and flux of dust in the coma, the dust fluence on a spacecraft along sample trajectories, and the radiation environment in the coma. The model will need to be refined when more details of the coma are revealed by observations. An overview of astronomical observations of 67P/C–G is given, because model parameters are derived from this data if possible. For quantities not yet measured for 67P/C–G, we use values obtained for other comets, e.g. concerning the optical and compositional properties of the dust grains. One of the most important and most controversial parameters is the dust mass distribution. We summarise the mass distribution functions derived from the in-situ measurements at comet 1P/Halley in 1986. For 67P/C–G, constraining the mass distribution is currently only possible by the analysis of astronomical images. We find that both the dust mass distribution and the time dependence of the dust production rate of 67P/C–G are those of a fairly typical comet.     

Comparison of magnetic flux tube and cosmic string behavior in Kerr metric

Cosmic strings are topological defects which were generated at a transition phase of the very early Universe and are probably responsible for large-scale structure forming. However, they may pull through all history and exist in the recent epoch. Thus, they can have influence for the recent Universe interacting with different objects. We consider the cosmic string behavior in the vicinity of a spinning black hole by means of a numerical simulation. Here we present preliminary results of this work via a comparison of cosmic string and magnetic flux tube behavior in the Kerr metric. Such an approach follows from the similarity of the equations which describe these objects. Therefore, many aspects of this behavior may be comparable.     

Frictional resistance of supercritical pressure RP-3 flowing in a vertically downward tube at constant heat fluxes

Based on the demands of compact heat exchangers and micro cooling channels applied for aviation thermal protection, the flow resistance characteristics of aviation kerosene RP-3 were experimentally studied in a vertically downward circular miniature tube with an inner diameter of 1.86 mm at supercritical pressures and constant heat fluxes. A long and short tube method was used to accurately calculate the frictional pressure drop, and experimental conditions are supercritical pressures of 4 MPa, mass flow rates of 2–4 g/s (i.e., mass fluxes of 736–1472 kg/(m²?s)), heat fluxes of 100–500 kW/m², and inlet temperatures of 373–673 K. Results show that the sharp variations of thermophysical properties, especially density, have significant influences on frictional resistances. Generally, the frictional pressure drop and the friction factor increase with increasing inlet temperatures, and this trend speeds up in the relatively high-temperature region. However, the friction factor has a sudden decline when the fuel outlet temperature exceeds the pseudo-critical temperature. The frictional pressure drop and the friction factor basically remain unchanged with increasing heat flux when the inlet temperature is relatively low, but increase quickly when the inlet temperature is relatively high. Besides, a larger mass flux yields a higher pressure drop but does not necessarily yield a higher friction factor. Finally, an empirical friction factor correlation is proposed and shows better predictive performance than those of previous models.     

Spaceborne quantitative assessment of dissolved organic carbon fluxes in the Kara Sea

An advanced algorithm for retrieval of phytoplankton chlorophyll (CHL) and dissolved organic carbon (DOC) concentrations from MERIS images of the Kara Sea is presented. The supply of DOC of terrestrial origin into the Kara Sea is numerically assessed from satellite data on DOC and historical records of river discharge rates. It exceeds the historical in situ values only by 25%. Satellite data on CHL were exploited for calculating the phytoplankton columnar biomass and the total phytoplankton biomass in the Kara Sea. Remote sensing and in situ data were used to calculate the value of the coefficient (K_PH) for calculation from phytoplankton biomass of autochthonous production of DOC. K_PH proved to be 142 ± 8 gC/gPH/month and exhibited only slight interannual variations. The coefficient K_PH was employed for the first time to evaluate the production of autochthonous DOC in the Kara Sea and to correct the value of the allochthonous DOC flux initially retrieved from space across the Kara Sea.     

滚动姿态对阳光与卫星向阳面夹角的影响分析

采用理论分析方法分析了卫星绕滚动轴滚动后,卫星向阳面与阳光的夹角的变化情况,用热分析工程软件NEVADA的数值计算反推结果,对理论分析结果进行了验证。分析结果表明：卫星姿态绕滚动轴滚动后,阳光与卫星向阳面的夹角相对于β角在不同纬度的变化趋势将不同,但在轨道周期内将发生周期性变化;随着滚动角的增大,该夹角的变化幅度也将增大。研究成果对卫星外热流分析具有参考意义。     

非均匀速度来流条件下液体射流喷雾特性

实验研究了非均匀速度来流条件下液体横向射流喷雾特性.实验利用多孔板实现速度的不均匀,应用片光照相得到喷雾中心截面照片,使用相位多普勒粒子分析仪(PDPA)测量液滴的直径和速度.实验结果表明:在非均匀速度来流中,射流的弯曲和破碎机理有所不同,导致穿透深度和雾化特性发生改变.与均匀速度来流相比,正速度梯度来流时射流穿透深度...     

证券市场资金流量模型研究

证券市场证券价格的运动可以划分为有明确趋势的定向运动与无趋势的随机波动。证券价格定向运动产生的内在原因及运动规律，是研究证券投资最关心的重要问题。文章以股票市场作为研究对象，从场内存量资金的定量分析着手，研究导致股价做定向运动的资金流量原理及其相关模型，得出资金进出股市“净流入（出）量”的测度方法履系列结论。     

建筑设计中的生态思维与对策

可持续发展问题是全人类共同面对的问题，该问题的核心又是人的行为与环境的关系问题，然而作为人类社会活动的重要组成部分，建筑在与环境的关系问题上长期以来走了一条弯路。如果情况再这样发展下去将会造成无法挽回的损失，扭转这种局面不仅是建筑师不可推卸的责任，也是时代向建筑师提出的挑战。要应对挑战，建筑师第一应具有清醒的头脑，第二还应掌握有效的方法。