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Fig. 14 EINO x versus 1000/T f of Comb 7 (from Mongia 2010a ) compared with the TFE731-2
data from Diehl and Biaglow ( 1974 ); the latter is identi ed as the first generation modern
propulsion engine and the former as N generation.
T f
is the adiabatic stoichiometric
flame
temperature computed from reported P 3 and T 3 data
stoichiometric
flame temperature), it is premature to recommend this approach for
all rich-dome engines to calculate the mission NO x emission. The similarity of these
two engines
fl
NO x versus stoichiometric curves and those in Fig. 13 discussed
earlier forces one to wonder how much rich-dome NO x reduction we can claim, and
therefore providing motivation for alternative design approaches.
Recalling from Fig. 13 , the takeoff NO x emissions of the set of several low rich-
dome combustors are represented well by a simple empirical correlation of their
takeoff pressure ratio. However, when the LTONO x data of these engines expressed in
terms of the average LTO NO x , the correlation quality deteriorates signi
'
cantly,
F 0 hi
namely DP
7319PR 0 : 9483
2
fit of these engines is
sought in terms of the characteristic LTO NO x (Fig. 15 ), the resulting expression is
worst off, namely DP
RD L ¼
1
:
w = R
¼
0
:
8459. When data
F 0 hi
6692PR 0 : 8552
2
RD L ¼
2
:
w = R
¼
0
:
6593
:
ning
RD-L, namely when it does not include the Trent1000 average LTO NO x . This is
obvious by looking at Fig. 15 which shows characteristic LTO NO x versus takeoff
However the quality of the empirical
fit improves considerably by rede
Fig. 15 Characteristic LTO
NO x of the lowest NO x rich-
dome large engines as de ned
in Fig. 13
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