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Direct numerical simulations of supercritical fluid mixing layers applied to heptane–nitrogen

Miller, Richard S. and Harstad, Kenneth G. and Bellan, Josette (2001) Direct numerical simulations of supercritical fluid mixing layers applied to heptane–nitrogen. Journal of Fluid Mechanics, 436 . pp. 1-39. ISSN 0022-1120. https://resolver.caltech.edu/CaltechAUTHORS:20171024-154826158

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Abstract

Direct numerical simulations (DNS) are conducted of a model hydrocarbon–nitrogen mixing layer under supercritical conditions. The temporally developing mixing layer configuration is studied using heptane and nitrogen supercritical fluid streams at a pressure of 60 atm as a model system related to practical hydrocarbon-fuel/air systems. An entirely self-consistent cubic Peng–Robinson equation of state is used to describe all thermodynamic mixture variables, including the pressure, internal energy, enthalpy, heat capacity, and speed of sound along with additional terms associated with the generalized heat and mass transport vectors. The Peng–Robinson formulation is based on pure-species reference states accurate to better than 1% relative error through comparisons with highly accurate state equations over the range of variables used in this study (600 ⩽ T ⩽ 1100 K, 40 ⩽ p ⩽ 80 atm) and is augmented by an accurate curve fit to the internal energy so as not to require iterative solutions. The DNS results of two-dimensional and three-dimensional layers elucidate the unique thermodynamic and mixing features associated with supercritical conditions. Departures from the perfect gas and ideal mixture conditions are quantified by the compression factor and by the mass diffusion factor, both of which show reductions from the unity value. It is found that the qualitative aspects of the mixing layer may be different according to the specification of the thermal diffusion factors whose value is generally unknown, and the reason for this difference is identified by examining the second-order statistics: the constant Bearman–Kirkwood (BK) thermal diffusion factor excites fluctuations that the constant Irwing–Kirkwood (IK) one does not, and thus enhances overall mixing. Combined with the effect of the mass diffusion factor, constant positive large BK thermal diffusion factors retard diffusional mixing, whereas constant moderate IK factors tend to promote diffusional mixing. Constant positive BK thermal diffusion factors also tend to maintain density gradients, with resulting greater shear and vorticity. These conclusions about IK and BK thermal diffusion factors are species-pair dependent, and therefore are not necessarily universal. Increasing the temperature of the lower stream to approach that of the higher stream results in increased layer growth as measured by the momentum thickness. The three-dimensional mixing layer exhibits slow formation of turbulent small scales, and transition to turbulence does not occur even for a relatively long non-dimensional time when compared to a previous, atmospheric conditions study. The primary reason for this delay is the initial density stratification of the flow, while the formation of strong density gradient regions both in the braid and between-the-braid planes may constitute a secondary reason for the hindering of transition through damping of emerging turbulent eddies.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0022112001003895DOIArticle
https://www.cambridge.org/core/journals/journal-of-fluid-mechanics/article/direct-numerical-simulations-of-supercritical-fluid-mixing-layers-applied-to-heptanenitrogen/A630F425D976534BC7291F626F2D347EPublisherArticle
https://doi.org/10.1017/S0022112002008625DOICorrigendum
Additional Information:© 2001 Cambridge University Press. Received 15 July 1999 and in revised form 16 November 2000. Published online: 22 June 2001. This research was conducted at the California Institute of Technology's Jet Propulsion Laboratory (JPL) while the first author was a Caltech Postdoctoral Scholar. Joint sponsorship was provided by General Electric (GE) through the Air Force Office of Scientific Research (AFOSR) Focused Research Initiative program with Dr Hukam Mongia from GE serving as contract monitor and by the National Aeronautics and Space Administration, the John Glenn Research Center at Lewis Field with Dr Daniel L. Bulzan as technical contract monitor. Computational resources were provided by the supercomputing facility at JPL. The constructive comments of one of the reviewers are acknowledged, prompting us to explore in more detail the various contributions to vorticity and vorticity magnitude production. The authors also wish to thank the Associate Editor, Professor S. K. Lele, for pertinent comments.
Errata:Owing to a printing error, figures 8, 9(a) and 9(b) are the same. Figure 8 is correct and the correct version of figure 9 is printed overleaf.
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Funding AgencyGrant Number
NASA/JPL/CaltechUNSPECIFIED
General ElectricUNSPECIFIED
Air Force Office of Scientific Research (AFOSR)UNSPECIFIED
Record Number:CaltechAUTHORS:20171024-154826158
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20171024-154826158
Official Citation:MILLER, R., HARSTAD, K., & BELLAN, J. (2001). Direct numerical simulations of supercritical fluid mixing layers applied to heptane–nitrogen. Journal of Fluid Mechanics, 436, 1-39. doi:10.1017/S0022112001003895
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:82636
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:24 Oct 2017 22:56
Last Modified:03 Oct 2019 18:56

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