Demarco Giuliano, Martins Luis Gustavo Nogueira, Bodmann Bardo Ernst Josef, Puhales Franciano Scremin, Acevedo Otávio Costa, Wittwer Adrian Roberto, Costa Felipe Denardin, Roberti Debora Regina, Loredo-Souza Acir Mércio, Degrazia Franco Caldas, Tirabassi Tiziano, Degrazia Gervásio Annes
Programa de Pós Graduação em Engenharia Mecânica, Universidade Federal de Santa Maria, Santa Maria 97105-900, Brazil.
Departamento de Física, Universidade Federal de Santa Maria, Santa Maria 97105-900, Brazil.
Int J Environ Res Public Health. 2022 Apr 23;19(9):5134. doi: 10.3390/ijerph19095134.
The aim of this paper is to analyse the thermal effects in a wind tunnel experiment to simulate the planetary boundary layer (PBL). Experiments were performed in the wind tunnel of the Laboratory of Constructions Aerodynamics at the Federal University of Rio Grande do Sul, Porto Alegre, Rio Grande do Sul State, Brazil. This wind tunnel is a closed return low-speed wind tunnel specifically designed for dynamic and static studies on civil construction models. As a novelty, one of the experimental sections of the wind tunnel was equipped with a metal sheet with Peltier elements coupled to it. In other words, thermal effects generating new flow patterns become feasible and open pathways to compare wind tunnel simulations to those in the PBL. Furthermore, measurements obtained with the smooth floor of the wind tunnel were repeated under the same conditions with the addition of the roughness in the floor, and the mechanical turbulence generated by the surface roughness significantly amplified the exchange of momentum and heat between the regions located in vertical direction of the wind tunnel boundary layer. In the presence of turbulent heat flux near the surface, thermal effects contribute to the increase of the turbulence intensity. Turbulent energy spectra for flow velocities and different heights were obtained using the Hilbert-Huang transform method, and the observed convective turbulence energy spectra behavior reproduced those measured in an unstable surface PBL.
本文旨在分析风洞实验中的热效应,以模拟行星边界层(PBL)。实验在巴西南里奥格兰德州阿雷格里港的南里奥格兰德联邦大学建筑空气动力学实验室的风洞中进行。该风洞是一个封闭式回流低速风洞,专门为土木建筑模型的动态和静态研究而设计。新颖之处在于,风洞的一个实验段配备了一块连接有珀耳帖元件的金属板。换句话说,产生新流动模式的热效应变得可行,并为比较风洞模拟与行星边界层中的模拟开辟了途径。此外,在风洞光滑地板的相同条件下,添加地板粗糙度后重复进行测量,表面粗糙度产生的机械湍流显著放大了风洞边界层垂直方向区域之间的动量和热量交换。在表面附近存在湍流通量的情况下,热效应有助于增加湍流强度。使用希尔伯特 - 黄变换方法获得了不同高度流速的湍流能量谱,观察到的对流湍流能量谱行为再现了在不稳定表面行星边界层中测量到的行为。