Geoscience Reference
In-Depth Information
Tabl e 8. 1
Correlation functions associated with the power approximations ( 8.10 ) of the Gaussian
CF in
and 3 are rewritten in terms of elementary functions
for convenience. The correlation radius adjustment coefficients
n
dimensions. The CFs for
n D 1
m are shown below the formulas
e m in approximation of the Gaussian CF (bold
together with the corresponding relative errors
numbers)
n D 1
n D 2
n D 3
m D 1
. /
K 0 ./
. /=
exp
exp
p
0.33
m D 2
.1 C /
. /
K 1 ./
. /
exp
exp
p 2
p =2
p 8=
0.13
0.19
0.33
.1 C C 2 =3/ exp . /
2 K 2 ./=2
m D 3
.1 C / exp . /
p
p 16=3
p 3=4
27=8
0.08
0.10
0.13
8.2.3
The Inverse Polynomial Model
A certain disadvantage of the binomial models ( 8.9 )and( 8.10 ) is their inability to
represent oscillating CFs whose spectra may have multiple maxima. This issue can
be overcome by considering the BEC models of the form:
2
3
1
J X
4 I C
a j D j
5
B D
(8.19)
j D 1
Here
a j are the real numbers, constrained by the positive definiteness requirement
of B . In the Fourier representation, the operator ( 8.19 ) acts as multiplication by the
inverse of the polynomial in
k 2 , and the positive-definiteness property translates into
the requirement that the spectral polynomial
J X
B 1 .k 2 / D 1 C
a j . k 2 / j
(8.20)
j D 1
k 2 >0
should be positive for all
. This constraint is equivalent to the statement that
the rhs of ( 8.20 ) must not have real positive roots. Therefore,
B 1 .k 2 /
can also be
represented in the form
Y
B 1 .k 2 / D 1
Z
.k 2 C z 2 m /.k 2 C z 2 m /;
(8.21)
m D 1
where
M D J=2
,
Z D Y
m
j z 2 m j 2 ;
(8.22)
 
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