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M
S
1
S
2
Fig. 10.8
According to the model by Dudkin et al. (
2010
), the magnetic dipole vector
M
is on the
intersection line of polarization ellipse planes measured at two different ground-based station, S
1
and S
2
z
1
y
1
y
z
O
1
x
1
M
z
2
l
1
O
x
y
2
M
l
2
O
2
x
2
M
y
z
z
'
r
0
ʸ
p
m
ʱ
1
Earthquake
focal zone
x
ʱ
2
Fig. 10.9
A sketch of equipment arrangement and the magnetic-dipole source location. The
reference magnetometer is located at the origin of coordinate system O, and the places of the
second and third magnetometers are shown by the vectors
l
1
and
l
2
Semi-empirical and semi-analytic techniques for finding the ULF source in
the background of natural noise have been reported by Surkov et al. (
2004
).
To distinguish a weak ULF source signal from the natural noise, a network of
multicomponent magnetometers is supposed to be used. A sketch of equipment
arrangement is shown in Fig.
10.9
. The distances between magnetometers are
designed such that
j
l
1
j
,
j
l
2
j
L, where L is the spatial scale of the variations
originated from the ionosphere-magnetosphere origin. The influence of these large-
scale variations can be eliminated by subtraction of data measured by a set
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