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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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