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Corynebacterium glutamicum - JUWEL - Forschungszentrum Jülich

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2. Theory<br />

evaluation can be made by comparing the achieved ˜χ 2 with values from standard chi<br />

squared tables. The strict use of this rule might be difficult for dynamic fermentation<br />

processes. Often, models are used with success although they probably do not meet the<br />

chi squared rule. As also discussed in paragraph 2.2 on page 9, a severe simplification of<br />

the complex system has to be made in order to get models which might be suitable for<br />

process optimization and control. Furthermore it is often difficult to estimate the real<br />

standard deviation of some of the measurements. The real measurement error of dilution<br />

steps and the measurement equipment can usually easily be determined. Possible errors<br />

by non-homogeneous samples, time delays in the off-line measurements et cetera, may<br />

be more difficult to estimate. These errors can cause higher standard deviations and a<br />

relatively high amount of outliers. Therefore, the choice of whether to reject a model is<br />

usually not done solely based on a little bit too high a ˜χ 2 . Still the reduced chi squared<br />

value forms a very valuable quantitative measure for the goodness of the fit and can also<br />

be used to compare the fit of different models. The weighting by the degree of freedom<br />

in the reduced form of the chi squared value provides some favouring of more simple<br />

models with less parameters.<br />

By using the reciprocal of ˜χ 2 , so that higher values represent better fits, and by<br />

subsequent scaling of the values for all m compared models to 1, a measure of the<br />

relative goodness of fit of different models can be calculated. So, the measure Gi for<br />

model i can be calculated as:<br />

Gi =<br />

1<br />

˜χ 2 i<br />

m�<br />

i<br />

1<br />

˜χ 2 i<br />

(2.35)<br />

Another method of comparing the fits of competing models is the Bayes approach<br />

of calculating relative model probabilities as mentioned for instance by Box and Hill<br />

(1967) or discussed by Stewart et al. (1996, 1998). Assuming a normal distribution of<br />

the measurement error, they formulated the probability density function pi of a model<br />

prediction ˆyi,n according to model i and measurement n as<br />

�<br />

�<br />

pi,n =<br />

1<br />

�<br />

2π(σ 2 + σ 2 i,n )<br />

exp<br />

−<br />

1<br />

2(σ2 + σ2 2<br />

− ˆyi,n)<br />

i,n )(y<br />

(2.36)<br />

where σ2 is the variance of the measured value and σ2 i,n is the variance of the model<br />

prediction. This last variance is also called the model variance, which is the term that<br />

will be used further in the current work. This model variance is described in more detail<br />

in paragraph 2.5.1 on page 26.<br />

Then, the relative probability of model i out of m competing models after n measurements<br />

is calculated as<br />

Pi,n−1 · pi,n<br />

Pi,n = �m i=1 Pi,n−1<br />

. (2.37)<br />

· pi,n<br />

20

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