{"title":"Examination of the onset and decay of turbulence in pipe flow","authors":"Basheer A. Khan, Shai Arogeti, Alexander Yakhot","doi":"10.1103/physrevfluids.9.093903","DOIUrl":null,"url":null,"abstract":"The crisis (or critical) Reynolds number (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mtext>Re</mtext><mi>c</mi></msub></math>) is established at 1870, describing the threshold beyond which the lifetimes of turbulent puffs prior to the relaminarization extend from <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>O</mi><mrow><mo>(</mo><msup><mn>10</mn><mn>4</mn></msup><mo>)</mo></mrow><mspace width=\"0.16em\"></mspace><mtext>to</mtext><mspace width=\"0.16em\"></mspace><mi>O</mi><mrow><mo>(</mo><msup><mn>10</mn><mn>6</mn></msup><mo>)</mo></mrow></mrow></math> time units (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mi>D</mi><mo>/</mo><msub><mi>U</mi><mi>m</mi></msub></mrow></math>), where <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>D</mi></math> and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>U</mi><mi>m</mi></msub></math> denote the pipe diameter and mean velocity, respectively. To analyze the role of inplane motion for sustaining turbulence, fully resolved direct numerical simulations have been performed to generate a localized, equilibrium turbulent puff at <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mtext>Re</mtext><mo>=</mo><mn>1920</mn></mrow></math>. Employing our approach based on proper orthogonal decomposition, the research confirms that azimuthal motion significantly contributes to the transition to turbulence. Notably, at supercritical Reynolds numbers (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mtext>Re</mtext><mo>></mo><msub><mtext>Re</mtext><mi>c</mi></msub></mrow></math>) ranging from <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mtext>Re</mtext><mo>=</mo><mn>1920</mn></mrow></math> to <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mtext>Re</mtext><mo>=</mo><mn>2100</mn></mrow></math>, reducing azimuthal motion energy by 80% substantially shortens the lifetime of turbulent puffs. It has been shown that the relaminarization of turbulent puffs at subcritical Reynolds numbers, <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mtext>Re</mtext><mo>=</mo><mn>1720</mn><mtext>–</mtext><mn>1840</mn></mrow></math>, clearly implies an exponential time decay of turbulence energy. The expression for the decay rate was obtained as a best-fit curve of direct numerical simulations.","PeriodicalId":20160,"journal":{"name":"Physical Review Fluids","volume":"14 1","pages":""},"PeriodicalIF":2.5000,"publicationDate":"2024-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review Fluids","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevfluids.9.093903","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, FLUIDS & PLASMAS","Score":null,"Total":0}
引用次数: 0
Abstract
The crisis (or critical) Reynolds number () is established at 1870, describing the threshold beyond which the lifetimes of turbulent puffs prior to the relaminarization extend from time units (), where and denote the pipe diameter and mean velocity, respectively. To analyze the role of inplane motion for sustaining turbulence, fully resolved direct numerical simulations have been performed to generate a localized, equilibrium turbulent puff at . Employing our approach based on proper orthogonal decomposition, the research confirms that azimuthal motion significantly contributes to the transition to turbulence. Notably, at supercritical Reynolds numbers () ranging from to , reducing azimuthal motion energy by 80% substantially shortens the lifetime of turbulent puffs. It has been shown that the relaminarization of turbulent puffs at subcritical Reynolds numbers, , clearly implies an exponential time decay of turbulence energy. The expression for the decay rate was obtained as a best-fit curve of direct numerical simulations.
期刊介绍:
Physical Review Fluids is APS’s newest online-only journal dedicated to publishing innovative research that will significantly advance the fundamental understanding of fluid dynamics. Physical Review Fluids expands the scope of the APS journals to include additional areas of fluid dynamics research, complements the existing Physical Review collection, and maintains the same quality and reputation that authors and subscribers expect from APS. The journal is published with the endorsement of the APS Division of Fluid Dynamics.