Geoscience Reference
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Fig. 10.6
P p )of
the posterior error to the
prior projected in data-space.
The overfit ( black ) method
generates a higher error
estimate compared to the
constrained ( grey ) method
across all choices of
background and observational
errors as well as over varying
numbers of observations
Ratio ( P a =
3 Obs
12 Obs
1
0.95
0.9
0.85
0.8
0.75
0.7
0.65
0.6
0.55
0.5
0.2
0.4
0.6
0.8
1
1.2
1.4
1.6
1.8
2
P
Fig. 10.7 Comparison of
prior R and posterior R a
observational error for overfit
( black ) and constrained ( grey )
methods
3
2.5
2
1.5
1
0.5
0
0
0.5
1
1.5
2
2.5
3
R
the observations. The constrained method slightly underestimates the observational
error, but is consistent with the prior . This exposes the overfit method for placing
too much emphasis on the observations.
As a final comparison, the theoretical cost-function minimum is compared to the
minimized cost-function at the end of each outer-loop. Because the overfit method
is unconstrained by P after the first outer-loop, it was shown that it will minimize
J o at the expense of
J b .
Bennett ( 2002 ) showed that for correctly specified P and R , the minimum value
of the cost-function is
. This measure has been used as a useful
diagnostic by Weaver et al. ( 2003 )and Powell et al. ( 2008 ). Unfortunately, this
measure does not quantify the contribution of each component of the cost function.
Moore et al. ( 2011a ) provides a concise review of the work of Talag r an d ( 1999 ),
Chapnik et al. ( 2006 ), and Desroziers et al. ( 2009 ) along with the derivation for
determining the minimum theoretical values of each cost-function component. The
J min D N obs =2
 
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