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 Encyclopedia of Physical Science and Technology  En006G-249  June 27, 2001  14:7







               60                                                                        Fluid Dynamics (Chemical Engineering)


               The actual velocity field fluctuates wildly. Reynolds mod-  mean values. Thus, any solution of Eq. (10) for the stress
               eled it by a superposition of a Eulerian time mean value ¯ v  distribution also becomes a solution of Eq. (124) for the
               defined by                                         “turbulent” stress distribution. Howe ver, this small suc-

                                   1     t                       cess extracts a dear price. No further progress can be made



                           ¯ v(x, t) =  v(x, t ) dt ,   (121)    because a new unknown quantity, ρv v , which has come
                                   t  0                          to be known as the Reynolds’ stress tensor, has been intro-
               where t is a time interval of the order of an individual  duced with no compensating new equation for its calcula-

               excursion and t is a time interval large in comparison with  tion. This is the famous turbulence “closure” problem.

               t but small enough that gross time variations of the mean  An enormous amount of effort has been expended in at-
               field can still be observed and calculated by the basic field  tempting to discover new equations for ρv v . Five differ-

               equations. In terms of this model then, we write  ent levels of approach have been pursued in the literature
                                                                 involvingvariousdegreesofmathematicalcomplexity.We

                                  v = ¯ v + v           (122)
                                                                 cannot discuss all of them here. We outline only two of
               with ¯ v being the instantaneous excursion or “fluctuation”  the most fruitful: (1) the mixing length or zero-equation

               from ¯ v. After this result is introduced into the field equa-  models and (2) the κ–ε or two-equation models.
               tionsandthetime-averagingoperationdefinedinEq.(121)
               is invoked, we obtain a new set of averaged field equations
               for the turbulent flow.                            C. Mixing Length Models
                 For incompressible fluids we obtain the following re-  An early approach to the closure, typified by the work of
               sults:                                            Prandtl, represented the Reynolds’ stress tensor as
                 Equation of Continuity
                                                                                              ¯

                                                                                 ρv v = 2ρˆ  τ · D,        (129)
                                  ∇ · ¯ v = 0           (123)
                                                                                                              ¯
                                                                 where ˆ  τ is a second-order eddy diffusivity tensor and D
                 Cauchy’s Equations of Motion
                                                                 is the symmetric part of ∇¯ v defined by Eq. (37) for v = ¯ v.
                     D¯ v                                        In this degree of approximation ˆ  τ is assumed to depend
                    ρ    + ∇ · ρv v = ρg − ∇ ¯ p − ∇ · ¯τ  (124)

                      Dt                                         only on the properties of the mean velocity gradient tensor
                                                                  ¯
                 Thermal Energy Relation                         D and is
                         ∂ ¯ u
                        ρ   + ρ¯v · ∇¯ u + ρv · ∇u                             ˆ   τ = 2L  2    −2II ¯ D |δ,  (130)

                          ∂t
                            τ


                        =− ¯ :∇¯ v − τ :∇v − ∇ · ¯ q + ˙ r CR  (125)  where L is some sort of length measure of the turbulence
                                                                                           is defined by Eq. (38) for
                                                                 called a mixing length, and II ¯ D
                 Mechanical Energy Relation
                                                                 v = ¯ v.
                             2
                                            2
                     ρ(∂/∂t)(¯v /2) + ρ(∂/∂t)(v /2) + ρ¯ v¯ v : ∇¯ v  For the special case of pipe flow, Prandtl modeled L as
                       + ρ¯ vv : ∇v + ρv ¯ v : ∇v + ρv v : ∇¯ v                   L = k t R(1 − ξ),        (131)





                       + ρv v : ∇v = ρ¯ v · g − ¯ v · ∇ ¯ p


                                                                 where k t , known as the Von Karman constant, is an em-
                       − v · ∇p − ¯ v · (∇ · ¯τ) − v · (∇ · τ )  (126)  pirical parameter usually taken to be ∼0.36. This simple




                                                                 model leads to a rather famous results for the velocity
                 Entropy Production Postulate
                                                                 distribution in a pipe:
                            − ¯τ :∇v − τ :∇v ≥ 0        (127)


                                                                               1
                                                                   +      ∗          +            +
                                                                  u = v/v =       ln y + 3.80,   y > 26    (132)
                 All of these relations contains terms involving statistical  0.36
               correlations among various products of fluctuating veloc-
                                                                        Rv ρ
                                                                          ∗
                                                                   +
               ity, pressure, and stress terms. This renders them consid-  y =  (1 − ξ)                    (133)
               erably more complex than their laminar flow counterparts.  µ
               Reynolds succeeded in partially sol ving this dilemma by  ∗
                                                                   v =   τ w /ρ                            (134)
               the expedient of introducing the turbulent stress tensor ˆτ,
               defined by                                         The dimensionless variables u +  and y +  are called
                                                                 Prandtl’s universal velocity profile variables. The

                                ˆ τ = ¯τ + ρv v .       (128)
                                                                 parameter v is called the friction velocity.
                                                                           ∗
               With this substitution Eq. (124) becomes identical with  In efforts to increase the range of applicability of the
               Eq. (10), with all terms replaced by their Eulerian time  mixing length model, numerous others have modified it.
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