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arXiv 2401.03032physics.flu-dyn
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相互作用的新月形沙丘上湍流流动的数据集

Dataset of turbulent flow over interacting barchan dunes

Jimmy Gabriel Alvarez, Danilo da Silva Borges, Erick de Moraes Franklin

AI总结:

本文提供了一个关于水下孤立或相互作用新月形沙丘上湍流流动的实验数据集,通过PIV和PTV技术测量流场,包含平均流场、轨迹、二阶矩及原始数据,可用于基准测试和新图像处理。

摘要:

新月形沙丘是常见于地球、火星和其他天体沙丘场中的沙丘,它们在那里可以相互发生作用。本文涉及水下新月形沙丘上方流动的实验数据,这些沙丘要么是孤立的,要么是相互作用的。实验在一个矩形截面的透明通道中进行,其中湍流水流被施加在单个或一对新月形沙丘上。瞬时流场通过使用低频PIV(粒子图像测速)和高频PTV(粒子追踪测速)进行测量。从PIV和PTV数据中,计算了平均流场、轨迹和二阶矩,这些内容连同原始数据(图像)、瞬时场和处理它们的脚本一起包含在本文描述的数据集中。这些数据集可被重新用于基准测试或处理由其他研究团队生成的新图像。

英文摘要:

Barchans are dunes commonly found in dune fields on Earth, Mars and other celestial bodies, where they can interact with each other. This article concerns experimental data for the flow over subaqueous barchans that are either isolated or interacting with each other. The experiments were carried out in a transparent channel of rectangular cross section in which turbulent water flows were imposed over either one single or a pair of barchans. The instantaneous flow fields were measured by using a low-frequency PIV (particle image velocimetry) and high-frequency PTV (particle tracking velocimetry). From the PIV and PTV data, the mean flow, trajectories, and second-order moments were computed, which are included in the datasets described in this paper, together with raw data (images), instantaneous fields, and scripts to process them. The datasets can be reused for benchmarking or for processing new images generated by other research groups.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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