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)
+ 1 1
1 + 1
a 2 cos
E y (
r cos
for
r
a
r
U ( r
, ,
)
=
(7
.
1)
1
1 + 1
2
E y (
)
r cos
for
r
a
,
where E y (
) is the normal electric field on the Earth's surface z
=
0 (Smythe,
1950). The function U satisfies the boundary conditions
=+ 0 0 =
r = a + 0 =
r = a 0 .
U
1
U
1
1
U
0
U | r = a + 0 =
U | r = a 0
r
r
On differentiating U , we get the electric field along the y -axis:
= 0
=−
U ( r
, ,
)
E y ( y
,
)
=
E y ( y
,
z
=
0
,
)
r
1
E y (
+ 1 1
1 + 1
a 2
y 2
(7
.
2)
)f r
|
y
| ≥
a
=
1
1 + 1
2
E y (
|
|
)
for
y
a
,
whence
1
Z N (
+ 1 1
1 + 1
a 2
y 2
)f r
|
y
| ≥
a
E y ( y
,
)
Z ( y
,
)
=−
=
(7
.
3)
2
1 + 1
2
H x
Z N (
)
for
|
y
| ≤
a
,
where H x
E y /
H x
is the normal magnetic field on the Earth's surface and Z N
=−
is the normal impedance.
Thus,
1
2
+ 1 1
1 + 1
a 2
y 2
Z ( y
)
= N (
N (
)
)f r
|
y
| ≥
a
2
,
( y
,
)
=
=
2
2
o
1
1 +
=
N (
)
N (
)
for
|
y
| ≤
a
,
.
(7
4)
2
,
where
= | Z N |
/ 0 is the normal apparent resistivity and
are the real
N
frequency-independent distortion factors
1
2
1
1
a 2
y 2
2
=
, =
1
+
.
(7
.
5)
1
1
1 +
1 +
1
1
 
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