热管翘片的优化设计

理论分析提出翘片传热效率的概念,推导翘片厚度、翘片高度和翘片的间距或者系数x决定了传热效率,也就是强化传热的效果。在翘片材料为黄铜、强制对流条件下,分析了优化翘片各参数,提出临界翘片厚度的概念,给出临界翘片厚度和翘片高度的关系曲线。     

应用UBET优化开式模锻中连皮厚度参数

连皮厚度是开式模锻工艺参数中的一个重要参量，它对模锻变形力和材料的消耗有很大的影响。本文应用上限单元法（ＵＢＥＴ）对连皮厚度进行了优化设计。基于连皮厚度和飞边高度间的相对大小关系，建立了三种不同的变形流动模式和动可容速度场，根据上限原理和黄金分割法，利用ＴｕｒｂｏＣ语言编程求解，获得了最大锻造力的最佳上限解，并和实验相比较，两者吻合得较好，表明建立的动可容速度场是合理可行的。以最大锻造力和连皮体积的乘积作为优化准则，更好地得到了最佳连皮厚度值。     

物证DNA分析技术的过去与现在

使用DNA指纹鉴定技术不仅可得到可靠的否定结论,还可以得到可靠的认定结论.PCR技术极大地提高了检测生物检材的灵敏度.借助芯片技术可一次性对样品大量序列进行实时、灵敏、精确地检测和分析.从第一代分析方法应用于法庭科学开始,第二、第三代分析技术的诞生以及相继应用,使个人识别及亲子鉴定的结果愈来愈精确.     

Validation of University of New Brunswick Ionospheric Modeling Technique with ionosonde TEC estimation over South Africa

For more than a decade, ionospheric research over South Africa has been carried out using data from ionosondes geographically located at Madimbo (28.38°S, 30.88°E), Grahamstown (33.32°S, 26.50°E), and Louisvale (28.51°S, 21.24°E). The objective has been modelling the bottomside ionospheric characteristics using neural networks. The use of Global Navigation Satellite System (GNSS) data is described as a new technique to monitor the dynamics and variations of the ionosphere over South Africa, with possible future application in high frequency radio communication. For this task, the University of New Brunswick Ionospheric Modelling Technique (UNB-IMT) was applied to compute midday (10:00 UT) GNSS-derived total electron content (GTEC). GTEC values were computed using GNSS data for stations located near ionosondes for the years 2002 and 2005 near solar maximum and minimum, respectively. The GTEC was compared with the midday ionosonde-derived TEC (ITEC) measurements to validate the UNB-IMT results. It was found that the variation trends of GTEC and ITEC over all stations are in good agreement and show a pronounced seasonal variation for the period near solar maximum, with maximum values (∼80 TECU) around autumn and spring equinoxes, and minimum values (∼22 TECU) around winter and summer. Furthermore, the residual ΔTEC = GTEC − ITEC was computed. It was evident that ΔTEC, which is believed to correspond to plasmaspheric electron content, showed a pronounced seasonal variation with maximum values (∼20 TECU) around equinoxes and minimum (∼5 TECU) around winter near solar maximum. The equivalent ionospheric and total slab thicknesses were also computed and comprehensively discussed. The results verified the use of UNB-IMT as one of the tools for future ionospheric TEC research over South Africa.     

An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation

An approach to inversion of the lunar regolith layer thickness by using multi-channel brightness temperature observation in passive microwave remote sensing is developed. To first make simulation of brightness temperature from the lunar layered media, the lunar regolith layer thickness (d) is proposed being constructed by available lunar DEM (digital elevation mapping) and on site measurements. The physical temperature distribution (T) over the lunar surface is also empirically assumed as a monotonic function of the latitude. Optical albedo of the lunar nearside from the telescopic observation is employed to construct the spatial distribution of the FeO+TiO₂ content (S) in the lunar regolith layer. A statistic relationship between the DEM and S of the lunar nearside is further extended to construction of S of the lunar farside. Thus, the dielectric permittivity (ε) of global lunar regolith layer can then be determined. Based on all these conditions (d,T,ε), brightness temperature of the lunar regolith layer in passive microwave remote sensing, which is planned for China's Chang-E lunar project, is numerically simulated by a parallel layering model using the strong fluctuation theory of random media.Then, taking these simulations with random noise as observations, an inversion method of the lunar regolith layer thickness is developed by using three- or two-channels brightness temperatures. When the S is low, and the four channels brightness temperatures in China's Chang-E project are well distinguishable, the regolith layer thickness and physical temperature of the underlying lunar rock media can be inverted by the three-channels approach. When the S becomes high that the brightness temperature at high frequency channels such as 19.35, 37 GHz are saturated, the regolith layer thickness is alternatively inverted only by the two-channels approach.Numerical simulation and inversion approach in this paper make an evaluation of the performance for lunar passive microwave remote sensing, and for future data calibration and validation.     

CMP加工过程中加工载荷对液膜厚度的影响分析

本文采用激光诱导荧光技术(LIF)来研究抛光参数对化学机械抛光加工区液膜厚度的影响.研究表明,抛光液膜厚度随着抛光载荷的增加而减少,减小的趋势随抛光载荷的提高而减缓.同时液膜厚度随着抛光速度的增加而变大.通过抛光参数的变化对抛光液液膜厚度影响的分析,为改善CMP加工工艺提供理论性的依据.     

聚酰亚胺泡沫吸声性能与理论分析

采用前驱体微球法制备闭孔聚酰亚胺泡沫,并对其吸声性能进行了研究。结果表明,闭孔聚酰亚胺泡沫具有共振吸声特点;对闭孔聚酰亚胺泡沫的吸声系数进行了理论推导,研究了泡沫厚度对泡沫吸声性能的影响,分析了聚酰亚胺泡沫的吸声理论;采用闭孔泡沫与开孔泡沫组合后,泡沫整体吸声性能显著提高。     

基于特征点的颅面复原技术

介绍了用人工神经网络算法确定待复原颅面的软组织厚度及颅面特征点的方法。在计算机辅助颅面复原过程中,通常只能根据颅骨上少数特征点及其所在部位的法向软组织厚度的统计值进行运算。由于现有统计值指标涵盖的年龄较宽泛,导致复原结果缺乏个性。在测定待复原颅骨骨龄的基础上,通过神经网络训练,确定软组织厚度随年龄的变化规律,较精确地计算出与拟复原对象的骨龄相适应的特征点软组织厚度值,并用最小二乘法及曲面法线原理建立数学模型,计算出颅面特征点。最后用基于Delaunay三角剖分的wavelet插值法复原出面貌雏形。     

高超声速飞行器热流密度/分层温度/碳化层研究

受试验设备能力限制,地面风洞无法完全模拟高超声速飞行器临近空间热环境。文章采用在飞行器表面开孔安装长时耐高温热流传感器直接测量热流密度的方法,国内首次获得Ma12以上高超声速飞行器表面热流密度时变数据和边界层转捩特征。实测热流值与理论预示值规律相同,两者偏差小于20%。针对树脂基材料导热微分方程中虽考虑了热解吸热项,但未考虑导热系数随温度变化情况,采用在树脂基材料导热微分方程中加入物性参数随温度变化项的方法,计算了飞行器热防护结构内部分层温度和碳化层厚度,并与实测结果进行了比较,不考虑树脂热解特性和材料物性参数随温度变化,理论值高于实测值,最大偏差275~320℃;考虑热解特性和物性参数随温度变化情况,计算值与实测值最大偏差小于70℃。     

尾缘厚度对低压涡轮气动性能影响的数值模拟

采用数值模拟的方法研究了尾缘厚度对Pak-B低压涡轮气动性能的影响.目的是通过增加尾缘厚度来控制边界层分离,降低损失,揭示增加尾缘厚度的流动控制机理.研究发现:适当增加尾缘厚度能减小低压涡轮损失,增大折转角.在雷诺数为25000,来流湍流度为1%时,适当增加尾缘厚度能使基于进口速度的能量损失系数降低10.4%,折转角增加1.73%.适当增加尾缘厚度和栅距同样可以使基于进口速度的能量损失系数减小,折转角增大.在雷诺数为25000,来流湍流度为1%时,尾缘厚度增加到4%s,栅距增加了2.2%,可以使基于进口速度的能量损失系数减小7.4%,折转角增加1.25%.通过增加尾缘厚度可以发展低稠度高负荷低压涡轮叶栅.