  <eprint id="http://authors.library.caltech.edu/id/eprint/284" xmlns="http://eprints.org/ep2/data/2.0">
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    <datestamp>2005-05-17</datestamp>
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      <item>
        <name>
          <family>Dimotakis</family>
          <given>Paul E.</given>
        </name>
        <id>Dimotakis-P-E</id>
        <uri></uri>
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    </creators>
    <title>Turbulent mixing</title>
    <ispublished>pub</ispublished>
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    <keywords>turbulence, entrainment, scalar dispersion, diffusion, reacting flow</keywords>
    <note>"Reprinted, with permission, from the Annual Review of Fluid Mechanics, Volume 37 copyright 2005 by Annual Reviews, www.annualreviews.org" &#xD;
&#xD;
Support for this reviewbyAFOSRGrants F49620&#x2013;01&#x2013;1&#x2013;0006 and FA9550&#x2013;04&#x2013;1&#x2013;0020, the DOE/Caltech ASCI/ASAP subcontract B341492, and the Caltech John K. Northrop Chair is gratefully acknowledged. I would also like to acknowledge both recent and previous discussions with and assistance by J. Adkins and W.R.C. Phillips on ocean mixing; D. Arnett, H. Bethe, and R. Lovelace on astrophysics and supernova explosions; J.E. Broadwell and M.G. Mungal on passive-scalar mixing; A.W. Cook, T.W. Mattner, D.I. Meiron, and P.L. Miller on RTI flow; H.J.S. Fernando, A. Mahalov, and J. Riley on mixing in stably stratified flows; H. Lam on scalar transport and diffusion; H.W. Liepmann on turbulence; C. Pantano on mixing and combustion dynamics; T.W. Mattner and D.I. Pullin on sub-grid scale modeling; and R.A. Shaw on particle and cloud dynamics; as well as assistance with the text by J.M. Bergthorson and D.I. Pullin.</note>
    <abstract>The ability of turbulent flows to effectively mix entrained fluids to a molecular scale is a vital part of the dynamics of such flows, with wide-ranging consequences in nature and engineering. It is a considerable experimental, theoretical, modeling, and computational challenge to capture and represent turbulent mixing which, for high Reynolds number (Re) flows, occurs across a spectrum of scales of considerable span. This consideration alone places high-Re mixing phenomena beyond the reach of direct simulation, especially in high Schmidt number fluids, such as water, in which species diffusion scales are one and a half orders of magnitude smaller than the smallest flow scales. The discussion below attempts to provide an overview of turbulent mixing; the attendant experimental, theoretical, and computational challenges; and suggests possible future directions for progress in this important field.</abstract>
    <date>2005</date>
    <date_type>published</date_type>
    <publication>Annual Review of Fluid Mechanics</publication>
    <volume>37</volume>
    <number>1</number>
    <pagerange>329-356</pagerange>
    <id_number>CaltechAUTHORS:DIMarfm05</id_number>
    <refereed>TRUE</refereed>
    <issn>0066-4189</issn>
    <official_url>http://resolver.caltech.edu/CaltechAUTHORS:DIMarfm05</official_url>
    <rights>You are granted permission for individual, educational, research and non-commercial reproduction, distribution, display and performance of this work in any format.</rights>
    <alt_url>http://dx.doi.org/10.1146/annurev.fluid.36.050802.122015</alt_url>
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