Geoscience Reference
In-Depth Information
200
0
60
latitude [deg]
Fig. 11.4.
Latitudinal dependency of the FLR-period
where
δ
i
is the half-width of the FLR-region in the ionosphere,
h
is the
E
-
layer height,
x
is the distance along the meridian,
x
r
(
f
) is the location of the
FLR. Coecient
C
1
is defined by the curvature of the FLR-line. It vanishes in
the 'box' model with a straight field (see Chapter 6). Such a model provides
reasonable accuracy with experimental data at
x
r
≤
500 km.
Let a half-width of an FLR-area on the ionospheric level be
δ
i
=20km.
Then a characteristic spatial scale of the resonance structure on the ground
is about 100-200 km. It is evident that there are geoelectrical cross-sections
for which the effective skin depth
d
g
in the
Pc
3
,
4 range and a horizontal field
scale are comparable. Therefore phase and amplitude features of the initial
waves noticeably influence the results of the magnetotelluric soundings of such
geological profiles.
Let
Φ, Λ
be the geomagnetic coordinates of an observation point. Assume
that the observed field at some frequency
f
results from FLR-oscillations of
the corresponding FLR-shell located at distance
180
π
from the observer. Here
Φ
r
(
f
) is the latitude of the FLR-shell with resonance
frequency
f
r
=
f
(see Fig.11.4). Latitude-dependence of FLR-frequency is
shown in Fig.11.4. The ground model is a four-layered geoelectrical cross-
section with
ρ
1
= 30 Ohm
x
r
(
f
) = 6370
·
(
Φ
r
(
f
)
−
Φ
)
·
10
3
Ohm
·
m
,h
1
=3km;
ρ
2
=3
×
·
m
,h
2
=
10
2
Ohm
50 km;
ρ
3
=3
m,
h
3
= 50 km and lower half-space with
ρ
4
=0
.
Ionospheric conductivities are
Σ
P
= 13 Ohm
−
1
,Σ
H
=14
−
1
Ohm
−
1
.
The height of the 'thin' ionosphere is
h
= 105 km. The calculations are
carried out for wavenumber
k
y
=0
.
Period
T
= 100 s is the FLR for the
geomagnetic latitude
Φ
=60
◦
. The dip is
I
=74
◦
. There were computed
×
·
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