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2)] S E S
1
2 [ R (
1
2 [ R (
H A
S 1 E R
=
π/
2)] J
=
π/
(1
.
82)
1
2 [ R (
[ h ] E R
S 1 [ I ]) E R
=
π/
2)] ( S [ e ]
=
,
where
1
2 [ R (
[ h ]
=
/
2)] ( S [ e ]
S 1 [ I ])
and [ R ], [ I ] are rotationl and identity matrices:
0
10
00
1
10
[ R (
/
2)]
=
,
[ I ]
=
.
Finally, with account for (1.68) and (1.70), we write
H S
[ h ] H R
=
,
(1
.
83)
where
[ h ][ Z R ]
=
+
.
.
[ h ]
[ I ]
(1
84)
The components of magnetic distortion tensor [ h ]are
1
2 ( Se yy
1
2 Se yx Z
S 1 ) Z
h xx =
1
+
h xy =−
(1
.
85)
1
2 Se xy Z
1
2 ( Se xx
S 1 ) Z .
h yx =−
h yy =
1
+
At the final stage, we go to (1.74) with (1.79), (1.80), (1.84) and synthesize the
LR-decomposition:
[ Z S ]
[ e ][ Z R ][ h ] 1
=
.
The truncated decomposition, [ Z S ]
[ e ][ Z R ] , is admissible if
=
2 ( Se yy
S 1 ) Z << 1
2 S e yx Z << 1
1
1
(1
.
86)
2 ( Se xx
S 1 ) Z << 1
2 S e xy Z << 1
1
1
.
The arithmetic suggests that near-surface magnetic anomalies can be neglected
in the period range T
>
2
·
,
100 s
providing S
300S and
1000 Ohm
m
h 2
, 3
·
.
100 km
100 Ohm
m
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