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= S 1 R 2 is the adjustment distance. The oscillation period L has a mean-
ing of the width of the structures. This critical parameter defines the intensity of
the S
where d
d , we have the narrow structures with barely perceptible
leakage of the excess current. Hence we observe here the strong S -effect with h
effect. As L << 2
π
S
and Q
d , we have the wide structures and the excess current in
the upper layer is barely perceptible due to the strong leakage. Hence we observe
here the weak S
1. As L >> 2
π
effect with h
<< S
and Q
0.
Figure 7.7 presents the L
dependence of Q . The strong S
effect with Q
exceeding 0.9 shows itself at L
2 d . The weak S
effect with Q
0
.
1 is observed
10 4
at L
20 d
.
Let
1
=
10 Ohm
·
m
,
h 1
=
1 km (sediments) and
2
=
Ohm
·
m
,
h 2 =
100 km (lithosphere). In this typical geoelectric situation we have the adjust-
ment distance d
effect is to be expected over the regional
structures (elevations, depressions) even 500-600 km wide.
Next
=
316 km and the strong S
we
examine
the
TE-mode.
It
is
represented
by
the
components
E x ( y
,
z )
,
H y ( y
,
z )
,
H z ( y
,
z ). On the surface of the perfectly conductive basement
E x ( y
,
h )
=
0
.
By virtue of (7.16)
E x ( y
,
0)
=
E x ( y
,
h 1 )
i
o h 1 H y ( y
,
0)
E x ( y
,
h 1 )
=−
i
o h 2 H y ( y
,
h 1 )
.
(7
45)
d 2 E x ( y
h 1
,
0)
H y ( y
,
0)
=
H y ( y
,
h 1 )
+
S 1 ( y ) E x ( y
,
0)
+
.
i
o
dy 2
Eliminating E x ( y
h 1 ) from these equations, we get the differential
relation between the electric and magnetic fields on the Earth's surface z
,
h 1 ) and H y ( y
,
=
0:
h 1 h 2 d 2 E x ( y )
dy 2
[1
i
o S 1 ( y ) h 2 ] E x ( y )
=
i
o hH y ( y )
,
(7
.
46)
Q
1
0.9
0.8
0.7
0.6
0.5
0.4
0.3
0.2
0.1
Fig. 7.7 Intensity of the
S -effect in relation to the
width of the structure L and
adjustment distance d
L/d
0
0
5
10
15
20
25
30
 
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