4.7 Article

Accelerating turbulence in heated micron tubes at supercritical pressure

期刊

JOURNAL OF FLUID MECHANICS
卷 972, 期 -, 页码 -

出版社

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2023.520

关键词

stratified turbulence; vortex breakdown; turbulence simulation

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This research focused on studying turbulent dynamics and heat transfer mechanisms in accelerating flows with variations in thermophysical properties and pressure drops in micron tubes. Direct numerical simulations were conducted to investigate the behavior of turbulence at supercritical pressure CO2 in heated micron tubes. The results showed that pressure drop and scale effect played important roles in the development of turbulence flows, leading to prominent property change and flow acceleration. The acceleration suppressed the production of turbulence and decreased heat transfer.
The purpose of this research was to provide further understanding of turbulent dynamics and heat transfer mechanisms in accelerating flows with thermophysical variations and pressure drops in micron tubes. Direct numerical simulations were conducted to investigate the turbulence to supercritical pressure CO2 in heated micron tubes with inner diameter 99.2 mu m. In general, the turbulent heat transfer enhancement/deterioration at supercritical pressure is dominated by variations in thermophysical properties, buoyancy and thermal acceleration; however, the mechanism differs in micron tubes (d* < 100 mu m). The results showed that the pressure drop and scale effect made significant contributions to the development of turbulence flows heated at supercritical pressure in micron tubes, leading to the prominent property change and flow acceleration in the inlet fully developed turbulent flow. The deviation on temperature distribution because of pressure changes was non-negligible. The primary contribution of the acceleration was the decay of a boundary layer, which significantly suppressed the production of turbulence and decreased heat transfer. The acceleration had stabilizing effects on the ejection and sweep motions of the turbulent flow. The high-speed fluid contributed to a new disturbance scenario of the flow with a larger spanwise wavenumber superimposed on existing perturbations. The high-speed streak width in the quasilaminar region was approximately 150-160v/u(tau) in accelerating flow. In the micron tubes, the Reynolds stress events of quadrant Q4 contributed 60 % of the Reynolds stress, greater than those of quadrant Q2.

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