基于DCOM技术构建分布式数控故障诊断系统

简要介绍DCOM技术的特点,对利用DCOM技术构建分布式数控故障诊断系统进行了研究,并提出了系统的组件模型结构。     

高职教育技能竞赛与课程群建设互动机制研究

高职教育技能竞赛和课程群建设间普遍存在着相互独立运行、沟通渠道不畅、缺乏促进机制等问题.针对上述问题,提出了在技能竞赛与课程群建设间建立良性互动机制的构想,设计了互动机制的循环反馈调节模型,分析了互动要素的驱动关系,给出了互动机制在课程群建设中的实现思路和操作方法.     

航空制件超声检测中的声场特性分析

 针对航空制件超声检测中影响缺陷定量准确性的声场问题进行了深入讨论, 研究了脉冲波声场的计算方法, 设计了相应的计算软件并绘制出实用换能器声轴线上的声压分布曲线, 分析了不同材料和厚度的采样回波对频谱的影响, 比较了连续波声场和脉冲波声场的分布特性及异同点。研究结果为提高超声检测中缺陷定量的准确性和科学性提供了依据。     

屈折形态学视角下的日语动词谓语的声调变化

在日语声调研究领域中,从屈折形态学的角度揭示日语动词谓语的声调变化规律,是一个崭新的声调研究视角。基于此,通过屈折形态学的研究方法,主要探讨了日语动词谓语发生形态变化时所引发的声调核移位现象以及其主要特征。日语动词谓语发生屈折形态变化时,随着语素的增加,声调核的位置也发生复杂的变化。如果从屈折形态学的视角分析日语动词谓语的声调变化,就能进一步挖掘声调变化的内在规律。     

关于多目标气动优化设计中伴随方法与对策理论的耦合研究(英文)

本文研究了多目标气动优化设计中伴随方法和对策理论的耦合问题,给出了伴随方法在每个对策策略中的具体应用和数值方法。在合作对策中伴随方法被并行地执行以共同得到Pareto阵面上的最优解;相反在Nash对策中伴随方法在Nash策略的最后被耦合起来以互相竞争的形式得到各自目标的最优解;而在Stackel-berg对策中伴随方法被分层耦合进"领头人"和"跟随者"的策略中以求解他们相互依赖的平衡解。文末的优化算例表明了本文耦合算法及其数值过程在求解多目标气动优化设计问题中的有效性。     

常开洞工业厂房风致内压试验研究

通过一系列不同条件下的单个常开洞单跨厂房刚性模型风洞测压试验,分析了风向角、开洞位置、开洞形状以及开洞大小对内压平均值与脉动值的影响,并与基于稳态理论与非定常理论的内压预测值进行了比较。研究发现,单个常开洞厂房内压的空间分布是均匀的,几乎处处相等,仅在开洞附近测点的风压系数值稍有差别;内压的脉动特性主要来源于来流湍流作用、旋涡脱落与尾流干扰以及赫姆霍兹共振等三个方面的影响;内压的均值与均方根值受开洞条件以及风向角等因素影响较大;稳态理论计算得到的内压系数均值与试验所得非常接近,但是均方根值的预测偏保守。非定常理论推导得到的内压响应方程在风速方向正对开洞时可以给出良好的预测,但由于受旋涡脱落、尾流干扰等影响,斜风向时运用该方法预测内压是不合适的。     

The Magnetic Field of Mercury

The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and observationally to distinguish the internal field from that due to the solar wind interaction. Conversely, the small field also means that Mercury offers an important opportunity to advance our understanding both of planetary magnetic field generation and magnetosphere-solar wind interactions. The observations from the Mariner 10 magnetometer in 1974 and 1975, and the MESSENGER Magnetometer and plasma instruments during the probe’s first two flybys of Mercury on 14 January and 6 October 2008, provide the basis for our current knowledge of the internal field. The external field arising from the interaction of the magnetosphere with the solar wind is more prominent near Mercury than for any other magnetized planet in the Solar System, and particular attention is therefore paid to indications in the observations of deficiencies in our understanding of the external field. The second MESSENGER flyby occurred over the opposite hemisphere from the other flybys, and these newest data constrain the tilt of the planetary moment from the planet’s spin axis to be less than 5°. Considered as a dipole field, the moment is in the range 240 to 270 nT-R _M ³ , where R _M is Mercury’s radius. Multipole solutions for the planetary field yield a smaller dipole term, 180 to 220 nT-R _M ³ , and higher-order terms that together yield an equatorial surface field from 250 to 290 nT. From the spatial distribution of the fit residuals, the equatorial data are seen to reflect a weaker northward field and a strongly radial field, neither of which can be explained by a centered-dipole matched to the field measured near the pole by Mariner 10. This disparity is a major factor controlling the higher-order terms in the multipole solutions. The residuals are not largest close to the planet, and when considered in magnetospheric coordinates the residuals indicate the presence of a cross-tail current extending to within 0.5R _M altitude on the nightside. A near-tail current with a density of 0.1 μA/m² could account for the low field intensities recorded near the equator. In addition, the MESSENGER flybys include the first plasma observations from Mercury and demonstrate that solar wind plasma is present at low altitudes, below 500 km. Although we can be confident in the dipole-only moment estimates, the data in hand remain subject to ambiguities for distinguishing internal from external contributions. The anticipated observations from orbit at Mercury, first from MESSENGER beginning in March 2011 and later from the dual-spacecraft BepiColombo mission, will be essential to elucidate the higher-order structure in the magnetic field of Mercury that will reveal the telltale signatures of the physics responsible for its generation.     

Research into Configuration and Flow of Wall Oil Film in Bearing Chamber Based on Droplet Size Distribution

The lubrication design and heat transfer determination of bearing chambers in aeroengine require a sufficient understanding of the oil droplet-film interaction and physical characteristic in an oil/air two-phase flow state.The analyses of oil droplet movement,mass and momentum transfer during the impingement of droplet/wall,as well as wall oil film thickness and flow velocity are very important for the bearing chamber lubrication and heat transfer calculation.An integrated model in combination with droplet movement,droplet/wall impact and film flow analysis is put forward initially based on the consideration of droplet size distribution.The model makes a contribution to provide more practical and feasible technical approach,which is not only for the study of droplet-film interaction and physical behavior in bearing chambers with oil/air two-phase flow phenomena,but also useful for an insight into the essence of physical course through droplet movement and deposition,film formation and flow.The influences of chamber geometries and operating conditions on droplet deposition mass and momentum transfer,and wall film thickness and velocity distribution are discussed.The feasibility of the method by theoretical analysis is also verified by the existing experimental data.The current work is conducive to expose the physical behavior of wall oil film configuration and flow in bearing chamber,and also significant for bearing chamber lubrication and heat transfer study under oil/air two-phase flow conditions.     

Mars Global Surveyor Observations of Solar Wind Magnetic Field Draping Around Mars

We examine the magnetic field in the martian magnetosheath due to solar wind draping. Mars Global Surveyor provided 3-D vector magnetic field measurements at a large range of altitudes, local times, and solar zenith angles as the spacecraft orbit evolved. We choose orbits with very clean signatures of draping to establish the nominal morphology of the magnetic field lines at local times of near-subsolar and near-terminator. Next, using a compilation of data from Mars Global Surveyor, we determine the average magnetic field morphology in the martian magnetosheath due to the solar wind interaction. The topology of the field is as expected from previous observations and predictions. The magnetic field magnitude peaks at low altitude and noon magnetic local time and decreases away from that point. The magnetic field has an inclination from the local horizontal of 5.6° on average in the dayside magnetosheath and 12.5° on the nightside. The inclination angle is closest to zero at noon magnetic local time and low altitude. It increases both upward and to later local times. The magnetic field in the induced magnetotail flares out from the Mars—Sun direction by 21°. Finally, we compare the observations to gasdynamic model predictions and find that the shocked solar wind flow in the martian magnetosheath can be treated as a gasdynamic flow with the magnetic pileup boundary as the inner boundary to the flow.     

冲击双层壁内通道表面换热系数的研究

为了研究双层壁内通道表面换热情况和冲击距离对换热影响,对双层壁结构内通道上、下表面的换热系数进行实验测量。由获得的换热系数来分析研究双层壁内部换热。并对冲击射流的机理作了分析。研究结果表明,在双层壁结构中,在高雷诺数时,在冲击板表面上会出现两个峰值;在进气板表面上也会出现位置随冲击高度变化的一高换热区;层板内通道表面上的换热系数随冲击距离的减小而增大。