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On the Formation of Nitrogen Oxides During the Combustion of ...

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5.2 <strong>Combustion</strong> <strong>of</strong> Partially Pre-Vaporized Droplets<br />

to diffusion (i.e. during homogenization, Fig. 5.12) and convection (i.e. <strong>the</strong> gas<br />

sampling process).<br />

Figure 5.13 depicts two trends <strong>of</strong> <strong>the</strong> NO x emissions over <strong>the</strong> pre-vaporization<br />

rate Ψ: If <strong>the</strong> correction factor f EINOx is taken into consideration, <strong>the</strong>re is no<br />

straightforward linear correlation <strong>of</strong> <strong>the</strong> emission index EI NOx (Ψ ≤ 0.5378),<br />

but it remains at a quasi-constant level. If <strong>the</strong> correction factor f EINOx is not<br />

taken into consideration, an almost linear decrease <strong>of</strong> EI NOx can be observed<br />

with an increase <strong>of</strong> Ψ, which is in compliance with Moesl et al. [296]. Fur<strong>the</strong>rmore,<br />

<strong>the</strong> corrected values <strong>of</strong> <strong>the</strong> NO x emissions are in good qualitative<br />

agreement with Figure 2.3 and 5.3 for sprays and single droplets, respectively.<br />

Thus, <strong>the</strong> experimental work at hand confirms <strong>the</strong> findings <strong>of</strong> <strong>the</strong> numerical<br />

simulations <strong>of</strong> Chapter 5.2: A substantial droplet pre-vaporization is required<br />

before NO x emissions can be reduced.<br />

The CO concentrations indicated by using <strong>the</strong> two FT-IR standards match<br />

perfectly for <strong>the</strong> lower Ψ-values and still very well for Ψ = 0.5378 (see also<br />

Fig. 5.13). This conformity was expected but is also an indication <strong>of</strong> high accuracy<br />

and data reproducibility <strong>of</strong> <strong>the</strong> exhaust gas analysis. The overall exponential<br />

increase in CO is due to <strong>the</strong> formation <strong>of</strong> a triple flame 4 with an<br />

increase in Ψ. The development <strong>of</strong> <strong>the</strong> triple flame is significantly triggered<br />

by <strong>the</strong> presence <strong>of</strong> a combustible gas phase along <strong>the</strong> droplet array and flame<br />

spread through this region as well as <strong>the</strong>rmal expansion <strong>the</strong>re<strong>of</strong>. While <strong>the</strong> degree<br />

<strong>of</strong> fuel vaporization Ψ increases, fuel-rich regions are gradually formed<br />

along <strong>the</strong> droplet array. These rich regions are consumed by <strong>the</strong> approaching<br />

triple flame, and thus tend to be an excessive source <strong>of</strong> CO production<br />

[211, 253, 344, 452]. This particular development <strong>of</strong> <strong>the</strong> triple flame structure<br />

was also confirmed through visual observation <strong>of</strong> <strong>the</strong> flame spread sequence<br />

(Fig. 5.14) and numerical work conducted by Kikuchi and coworkers<br />

[206, 208].<br />

Figure 5.14 shows sequences <strong>of</strong> flame spread associated with <strong>the</strong> emissions<br />

<strong>of</strong> <strong>the</strong> three experiment runs <strong>of</strong> Figure 5.13. The images are taken from highspeed<br />

recording and cover <strong>the</strong> field <strong>of</strong> view from <strong>the</strong> third to <strong>the</strong> fifth droplet.<br />

The flame front travels from left to right. In all cases, a dim blue flame marks<br />

<strong>the</strong> flame front, propagating into <strong>the</strong> unburned region. A yellow, luminous<br />

4 According to van Oijen and de Goey [452], a triple flame is a flame structure generated by flame propagation in<br />

a partially premixed system. Typical triple flames comprise a rich and lean premixed flame front and a diffusion<br />

flame, all <strong>of</strong> <strong>the</strong>m intercepting in <strong>the</strong> triple point. Triple flames are also denoted as tribrachial flames.<br />

177

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