基于效用价值驱动的旅客出行动力学研究与建模

为了探究交通体系中旅客出行行为的特征与机理,以某机场离港旅客的陆侧出行数据为研究对象,对旅客出行模式进行了统计。分析发现,旅客聚集行为具有强烈的阵发性,不同出行维度旅客群体的聚集时间间隔分布具有幂律特征,且幂指数和阵发性强度呈正相关关系。同时,研究认为旅客出行换乘决策是综合时间、费用、便捷舒适度、突发情况等多因素的期望实现,是一种基于效用价值驱动的人类行为。基于此构建了效用价值驱动模式下的旅客出行行为动力学模型,可输出幂指数为参数可调的幂律分布,且仿真输出和实证数据分析结果相吻合。      

临近空间环境下封闭方腔内耦合换热特性

以临近空间浮空器载荷舱为应用背景,对复杂热边界条件下含热源的三维封闭方腔内自然对流、表面辐射和导热的耦合问题进行了数值模拟。综合考虑对流换热、长波辐射、太阳辐射等因素的影响,建立了临近空间热环境模型。通过Fluent软件用户自定义函数（UDF）引入外部非定常的辐射-对流耦合热边界条件,对腔内换热特性的昼夜变化进行研究,并分析了腔壁厚度、发射率和导热系数对其的影响。数值结果表明,腔内平均温度昼夜变化很小,约为12.9 K,但温度场分布随太阳方位变化而变化;腔内对流换热较弱,同一时刻最大温差约为71.3 K;腔壁热阻和发射率增加会削弱自然对流的强度。      

结构形式对双层微通道热沉传热性能的影响

设计一种双层微通道热沉,即热沉上下层通道结构相异B（上层为矩形微通道,下层为复杂结构微通道）,旨在降低压降的同时保持良好的换热性能,并与上下层通道均为复杂结构微通道的热沉A作对比。用数值方法研究了顺流和逆流时、不同通道结构（PA、PB、CA、CB）对其传热性能的影响,并用场协同原理分析流场与温度场的协同关系对传热的影响。结果表明:当0相似文献   

R141b在矩形微尺度通道中的两相流传热特性

设计搭建水力直径分别为1mm和0.5mm的矩形微尺度通道实验台,研究了以R141b型制冷剂作为工质的两相流沸腾传热特性。实验取热流密度为1～16kW/m2、质量流速为111.1～333.3kg/(m2·s)和质量干度为0～1,分析了三者对平均传热系数的影响,探究影响换热的主导因素。结果表明:热流密度较高时,平均传热系数随热流密度增加而减小,流动换热主要受到沸腾传热的影响;当质量流速较大且热流密度较低时,平均传热系数随热流密度增加而有所增长;热流密度较低时,平均传热系数随质量流速变化明显,热流密度升高到一定值后,质量流速对平均传热系数的影响很小;当质量流速处于111.1～333.3kg/(m2·s)时,平均传热系数随质量干度的增加而减小。      

YE4系列超超高效率三相异步电动机效率验证的研究

IE4超超高效率为国际电工委员会发布的IEC 60034-30-1:2014标准中电动机的最高效率等级。采用B法——测量输入-输出功率的损耗分析法对YE4系列(IP55)三相异步电动机的各大损耗的精准测试,以及采用不同降耗设计措施所达效果等进行了实际验证,确保了全系列电机达到了IE4效率等级规定。YE4系列产品的成功开发及推广应用,将对进一步推进我国节能减排政策的落实做出重要的贡献。     

基于雷诺平均Navier-Stokes方程的表面传热系数计算

采用有限体积法数值求解控制二维绕流的雷诺平均Navier-Stokes(RANS)方程组,计算了光滑和粗糙NACA0012翼型以及圆柱表面的局部表面传热系数.分析了近壁面网格间距、湍流模式和表面粗糙度模型对数值计算结果的影响.结果表明:切应力输运(SST)湍流模型能够区分层流和湍流边界层的对流传热特性,并能预测转捩的发生;采用Spalart-Allmaras(S-A) 扩展模型能够计算粗糙壁面的对流传热系数,但采用忽略转捩函数的S-A模型不能有效计算层流边界层的传热系数.当近壁面网格间距接近10-5量级的黏性子层时,在光滑和粗糙壁面都能得到准确的传热系数分布.结合合适的近壁面网格间距,湍流模式和表面粗糙度模型可以得到与实验数据十分接近的表面传热系数曲线.通过与求解不可压缩RANS方程得到的结果比较后发现,不可压缩RANS方程主要忽略了压缩和黏性耗散效应,这种效应可以通过绝热升温项的形式并入总体热分析.      

汽雾两相流强化冷却燃气轮机叶片内冷通道

实验研究了方形通道这一重型燃气轮机中常用叶片强制对流冷却通道结构.分析了雷诺数、壁面热流密度以及水雾质量流量比等关键参数对汽雾冷却通道的传热特性的影响,并建立了考虑离散相水雾的流动工况和通道壁面加热条件的实验关联式.结果表明:相对于纯蒸汽,汽雾两相流的传热系数显著提高,且传热性能提高的幅度随热流密度的增大而减小,随雷诺数和水雾质量流量比的增大而增大;通道上壁面平均传热系数低于下壁面,在高热流密度和低水雾质量流量比下,两者相差约13%,而在低热流密度与高水雾质量流量比的情况下,该比值增加到约25%.      

Design of nanofluid-cooled heat sink using topology optimization

The paper presented topology optimization of 2D and 3D Nanofluid-Cooled Heat Sink (NCHS). The flow and heat transfer problem in the NCHS was treated as a single-phase nanofluid based convective heat transfer model. The temperature-dependent fluid properties were taken into account in the model due to the strong temperature-dependent features of nanofluids. An average temperature minimum problem was studied subject to the fluid area and energy dissipation constraints by using the density method. In the method, the design variable is updated according to the gradient information obtained by an adjoint based sensitivity analysis process. The effects of the energy dissipation constraint, temperature-dependent fluid properties and nanofluid characteristics on optimal configurations of NCHS were numerically investigated with following conclusions. Firstly, branched flow channels in the optimal configuration increased with the rise of the allowed energy dissipation. Secondly, temperature-dependent fluid properties were significant for obtaining the appropriate optimal results with best cooling performance. Thirdly, heat transfer performances of optimal configurations were enhanced by reducing the nanoparticle diameter or increasing the nanoparticle volume fraction. Fourthly, the optimal configuration for nanofluid had better cooling performance than that for its base fluid.     

Probing the origin of the iron Kα line around stellar and supermassive black holes using X-ray polarimetry

Asymmetric, broad iron lines are a common feature in the X-ray spectra of both X-ray binaries (XRBs) and type-1 Active Galactic Nuclei (AGN). It was suggested that the distortion of the Fe Kα emission results from Doppler and relativistic effects affecting the radiative transfer close to the strong gravitational well of the central compact object: a stellar mass black hole (BH) or neutron star (NS) in the case of XRBs, or a super massive black hole (SMBH) in the case of AGN. However, alternative approaches based on reprocessing and transmission of radiation through surrounding media also attempt to explain the line broadening. So far, spectroscopic and timing analyzes have not yet convinced the whole community to discriminate between the two scenarios. Here we study to which extent X-ray polarimetric measurements of black hole X-ray binaries (BHXRBs) and type-1 AGN could help to identify the possible origin of the line distortion. To do so, we report on recent simulations obtained for the two BH flavors and show that the proposed scenarios are found to behave differently in polarization degree and polarization angle. A relativistic origin for the distortion is found to be more probable in the context of BHXRBs, supporting the idea that the same mechanism should lead the way also for AGN. We show that the discriminating polarization signal could have been detectable by several X-ray polarimetry missions proposed in the past.