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impedances are defined from the magnetic field H y measured at a base station and
the filtered electric fields E fl x measured on the profile.
The low-frequency spatial filtering is performed by means of the Hanning trans-
formation (Bernard and Rader, 1969):
x 0 +
W
/
2
1
2
E flt
x
e x ( k x ) h ( k x ) e ik x x 0 dk x
( x 0 )
=
E x ( x ) H ( x
x 0 ) dx
=
π
x 0 W /
−∞
2
(11
.
10)
1
2
e fl x ( k x ) e ik x x 0 dk x ,
=
π
−∞
where H ( x ) is the Hanning window of width W :
1
1
W
cos 2
π
x
W
2
+
|
x
| ≤
W
H ( x )
=
W
2 ,
0
|
x
| >
h ( k x ) is its frequency response as a function of the spatial frequency k x :
1
e ik x x dx
W
/
2
1
W
cos 2
π
x
H ( x ) e ik x x dx
h ( k x )
=
=
+
W
−∞
W / 2
=
2
4
π
sin Wk x
2
Wk x
2
1
2
1
2
sin Wk x
2
Wk x
2
W 2 k x
=
1
1 ,
Wk x
Wk x
2
2
2
W 2 k x
4
π
1
+
1
e x ( k x ) is the spatial spectrum of the observed electric field E ( x ):
E x ( x ) e ik x x dx
e x ( k x )
=
,
−∞
and e fl x ( k x ) is the spatial spectrum of the filtered electric field E fl x ( x ):
e flt
x
( k x )
=
h ( k x )e x ( k x )
.
Figure 11.19 presents the filter using the Hanning windows. Its 3 dB cutoff point
with h
0
.
7 is located at Wk x
4
.
52. With increasing Wk x the amplitude falls as
( Wk x ) 3 .At Wk x
1
/
10
.
36 we have 20 dB attenuation with h
=
0
.
1.
The critical question is how to choose the optimum window width W . Bostick
(1984) believes that W should be proportional to the effective penetration depth h eff :
 
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