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Turbulent dissipation rate fluctuating

Models conditioned on the turbulent dissipation rate attempt to describe non-stationary effects due to the fluctuating strain-rate field, and thus should be adequate for flamelet applications which require a model for the mixture-fraction dissipation rate at the stoichiometric surface. [Pg.291]

The scalar dissipation rate acts as an external parameter that is imposed on the flamelet structure by the mixture fraction field [15]. It describes the influence of the turbulent flow field on the laminar flame stracture. Both the mixture fraction and the scalar dissipation rate fluctuate on turbulent flows, and their statistical distribution needs to be considered. If the joint pdf P Z, Xst) (where Xst is x at the stoichiometric condition) is known, the Favre mean of 7 can be obtained from... [Pg.95]

Pitsch H. Improved pollutant predictions in large-eddy simulations of turbulent non-premixed combustion by considering scalar dissipation rate fluctuations. Proc Combust Inst... [Pg.121]

The description is based on the previously defined single-particle (Lagrangian) or one-point (Eulerian) joint velocity-composition (micro-)PDF, /(r,yr). As mentioned in Section 12.4.1, in the one-point description no information on the local velocity and scalar (species concentrations, temperature,. ..) gradients and on the frequency or length scale of the fluctuations is included and the related terms require closure models. The scalar dissipation rate model has to relate the micro-mixing time to the turbulence field (see (12.2-3)), either directly or via a transport equation for the turbulence dissipation rate e. A major advantage is that the reaction rate is a point value and its behavior and mean are described exactly by a one-point PDF, even for arbitrarily complex and nonlinear reaction kinetics. [Pg.653]

In the RANS-approach, turbulence or turbulent momentum transport models are required to calculate the Reynolds-stresses. This can be done starting from additional transport equations, the so-called Reynolds-stress models. Alternatively, the Reynolds-stresses can be modeled in terms of the mean values of the variables and the turbulent kinetic energy, the so-called turbulent viscosity based models. In either way, the turbulence dissipation rate has to be calculated also, as it contains essential information on the overall decay time of the velocity fluctuations. In what follows, the more popular models based on the turbulent viscosity are focused on. A detailed description of the Reynolds-stress models is given in Annex 12.5.l.A which can be downloaded from the Wiley web-page. [Pg.662]

Turbulent dissipation rate of temperature fluctuation, s Variable, dimensionless Turbulent diflfusivity, no s ... [Pg.146]

Turbulent velocity fluctuations ultimately dissipate their kinetic energy through viscous effects. MacroscopicaUy, this energy dissipation requires pressure drop, or velocity decrease. The ener dissipation rate per unit mass is usually denoted . For steady ffow in a pipe, the average energy dissipation rate per unit mass is given by... [Pg.671]

The turbulent energy dissipation rate can be expressed in terms of the fluctuating rate-of-strain tensor ... [Pg.57]

Note that in the turbulent mixing literature, the scalar dissipation rate is often defined without the factor of two in (3.112). Likewise, in the combustion literature, the symbol X is used in place of in (3.112). In this book, we will consistently use to denote the fluctuating scalar dissipation rate, and = (e ) to denote the scalar dissipation rate. [Pg.105]

Given a stochastic model for the turbulence frequency, it is natural to enquire how fluctuations in co will affect the scalar dissipation rate (Anselmet and Antonia 1985 Antonia and Mi 1993 Anselmet et al. 1994). In order to address this question, Fox (1997) extended the SR model discussed in Section 4.6 to account for turbulence frequency fluctuations. The resulting model is called the Lagrangian spectral relaxation (LSR) model. The LSR model has essentially the same form as the SR model, but with all variables conditioned on the current and past values of the turbulence frequency [ /(. ),. v < r. In order to simplify the notation, this conditioning is denoted by ( , e.g.,... [Pg.341]

The maximum dissipation rates for the dispersion of droplets and gas bubbles with different stirrer types such as turbine and pitched-blade stirrers, Lightnin A 310 and Cheminer HE 3 was determined using ID-LDA measurements, and the resulting turbulent fluctuating velocities were calculated using a model based on dimensional analysis. The essential parameters were identified using statistical analysis supported by sensitivity analysis. It was found that in the relationship e oc the stirrer speed dependence with n is correct, but that for the stirrer diameter with was set too low. The number of baffles was of secondary importance [608]. [Pg.34]

The dissipation rate of the gas-particle fluctuation covariance Cgp and the gas-particle turbulent viscosity i/ are defined by ... [Pg.926]

Proper boundary conditions are generally required for the primary variables like the gas and particle velocities, pressures and volume fractions at all the vessel boundaries as these model equations are elliptic. Moreover, boundary conditions for the granular temperature of the particulate phase is required for the PT, PGT and PGTDV models. For the models including gas phase turbulence, i.e., PGT and PGTDV, additional boundary conditions for the turbulent kinetic energy of the gas phase, as well as the dissipation rate of the gas phase and the gas-particle fluctuation covariance are required. The... [Pg.927]

In turbulent flow, the streamlines are erratic and eddies occur. This leads to a strong mixing effect and to a greater energy dissipation rate. Flow is turbulent if the Reynolds number (proportional to flow velocity, channel dimension, and the inverse of viscosity) is greater than a critical value. Because of Bernoulli s law, which states that the sum of pressure and kinetic energy is constant, the strong velocity fluctuations in turbulent flow induce pressure fluctuations. These cause, in turn, inertial forces to act on any particles present. [Pg.151]


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See also in sourсe #XX -- [ Pg.52 ]

See also in sourсe #XX -- [ Pg.52 ]




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