Evaluation AC2-09

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SANDIA Flame D

Application Challenge AC2-09   © copyright ERCOFTAC 2024

Comparison of Test Data and CFD

In this section comparisons of the CFD results and test data are organized as follows:

  • Comparisons of two different approaches for modeling the turbulence/combustion interaction, namely: steady flamelet model and simplified Conditional Moment Closure (designated as CMC -model in the figures from here on) obtained with the classical Smagorinsky subgrid scale model,
  • Comparisons of two subgrid-scale models, namely: classical Smagorinsky subgrid scale model and dynamic Smagorinsky one using the steady flamelet model of turbulence/combustion interaction.

Fig.6. shows mean velocity axial component and mixture fraction along the centerline for both steady flamelet and CMC approaches. One can see quite significant discrepancies between both models. Steady flamelet shows rapid velocity decay in the near field and then the slope is quite close to the one measured experimentally. On the other hand the CMC model leads to much smaller velocity decay. The velocity profile for CMC is closer to experimental data but the slope at the distance z/D=10 is underpredicted. At the distance z/D=30 both models predict good velocity decay. As to the mixture fraction both models predict quite a long distance z/D ≤ 16 for which the mixture fraction is unity while the experiment showed much more intense mixing in this region. As a consequence, at the jet centerline for a distance z/D ≤ 16 the numerical models do not predict reaction and this is reflected in the temperature profile and combustion products like CO2 shown in Fig.8. However, further downstream in the fully developed flame the numerical results are much closer to the experimental data. Especially CMC predicts the value of temperature maximum and its location with quite high accuracy (see Fig.7).

AC2-09 fig6a.gif   AC2-09 fig6b.gif
Fig. 6. Axial velocity (left) and mixture fraction (right) along the flame axis
AC2-09 fig7.gif
Fig. 7. Temperature along the flame axis

The species distributions are shown in Figs 8-10. As the models predict the flame too far from the nozzle exit, in all species distributions similar discrepancies are observed at the distance z/D = 10 – 20. And again, as was observed for the temperature profile, further in the developed flame the agreement with experimental data is much better. The distributions for H2O, O2, CO predicted with CMC are nearly perfect. A bit worse results were obtained for H2.

AC2-09 fig8a.gif   AC2-09 fig8b.gif
Fig. 8. Mean mass fraction of CH4 (left) and CO2 (right)
AC2-09 fig9a.gif   AC2-09 fig9b.gif
Fig. 9. Mean mass fraction of H2O (left) and O2 (right)
AC2-09 fig10a.gif   AC2-09 fig10b.gif
Fig. 10. Mean mass fraction of CO (left) and O2 (right)

Fig.11 shows the fluctuating axial velocity and mixture fraction components. In the near field the velocity fluctuations predicted by both models at the distance z/D ≤ 10 are much higher than measured experimentally which is consistent with much faster velocity decay in this region shown in Fig.6. Further downstream in the developed flame, agreement is very good. For the fluctuating component of the mixture fraction shown in Fig.11 in the near field fluctuations are lower than observed experimentally and again in the developed flame agreement is quite good. Maximum value of temperature fluctuations (Fig.12) is located much closer to the nozzle exit than the maximum value of mean temperature. CMC leads to higher level of temperature fluctuations. Fluctuating components of major species are shown in Figs 13-15. Both models predict reasonable levels of species fluctuation in agreement with experimental results.

AC2-09 fig11a.gif   AC2-09 fig11b.gif
Fig. 11. RMS of axial velocity (left) and mixture fraction (right) along the jet flame axis
AC2-09 fig12.gif
Fig. 12. RMS of temperature along the jet flame axis
AC2-09 fig13a.gif   AC2-09 fig13b.gif
Fig. 13. RMS of mass fraction of CH4 (left) and CO2 (right)
AC2-09 fig14a.gif   AC2-09 fig14b.gif
Fig. 14. RMS of mass fraction of H2O (left) and O2 (right)
AC2-09 fig15a.gif   AC2-09 fig15b.gif
Fig. 15. RMS of mass fraction of CO (left) and H2 (right)

Sample radial profiles of mean and fluctuating velocities are shown in Figs 16 and 17. Both models predict radial velocity profiles in very good agreement with experiment in all the cross sections. Fluctuating components are also in good agreement with experimental data. At the last cross section at the distance z/D = 45 the flamelet model leads to some overprediction of fluctuating components far from the flame axis. Mean mixture fraction shown in Fig.18 is close to experimental data. As to the mixture fraction fluctuating component shown in Fig. 19 agreement with experimental data is also reasonable. However, a surprising result was obtained at the distance z/D = 30 where the radial distribution of fluctuating component of mixture fraction obtained with the CMC is qualitatively different from experimental profile and from the result obtained with steady flamelet. In the profile predicted with CMC a local maximum is observed on the axis that is not present in experimental data. At the current stage of the research it seems to be difficult to explain these discrepancies analyzing physics of turbulence/combustion interaction.

AC2-09 fig16a.gif AC2-09 fig17a.gif
AC2-09 fig16b.gif AC2-09 fig17b.gif
AC2-09 fig16c.gif AC2-09 fig17c.gif
Fig 16. Mean axial velocity radial profile at the cross sections (a) z/D=15, (b) z/D=30, (c) z/D=45 Fig 17. Fluctuating axial velocity radial profile at the cross sections (a) z/D=15, (b) z/D=30, (c) z/D=45
AC2-09 fig18a.gif AC2-09 fig19a.gif
AC2-09 fig18b.gif AC2-09 fig19b.gif
AC2-09 fig18c.gif AC2-09 fig19c.gif
Fig 18. Mean mixture fraction radial profile at the cross sections (a) z/D=15, (b) z/D=30, (c) z/D=45 Fig 19. Fluctuating mixture fraction radial profile at the cross sections (a) z/D=15, (b) z/D=30, (c) z/D=45




Contributed by: Andrzej Boguslawski — Technical University of Częstochowa

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© copyright ERCOFTAC 2024