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3
q=1.15
2.8
(1)
(2)
/f
r
f
r
2.6
l
2
(q,w
0
=0.8767)
2.4
2.2
2
0
1
2
3
4
5
6
q
Fig. 11.2.
Graphic calculation of (11.12)
concentration at the top of the field line
n
0
j
=
106
/Ω
j
L
j
2
= 226
.
9
,
273
.
7
,
321
.
2
,
390
.
3cm
−
3
.
The parameters
a
and
s
of the power approximation
(11.9) of the equatorial plasma density distribution are found from (11.18)
as
a
=3
10
3
cm
−
3
,
s
=1
.
767
.
The dependence of
n
0
on the geomagnetic latitude is shown in Fig. 11.3.
The solid circles in Fig. 11.3 are calculated according to (11.15). The approx-
imation (11.9) is shown with the line.
The obtained values of plasma concentration
n
0
,
and the parameters
q
and
s
are in good agreement with those obtained from the satellite and whistler
measurements under weak and moderate geomagnetic activity at
L
= 3-4
(e.g., [11], [27], [31]). The analysis of the accuracy of the estimates of plasma
density with hydromagnetic diagnostics [15] shows that the accuracy of this
method is close to that of whistler measurements [28]. Besides, the MHD-
diagnostics combined with whistler measurements allow us to estimate the
concentration of heavy ions in the magnetosphere.
×
11.3 Ground-Based Magnetotelluric Sounding
Impedance
The horizontal electric and magnetic field components on the ground are
linked by a linear operator
Z
which is a functional from the distribution of
the ground conductivity
σ
g
(
r
). For a layered medium providing the basis
for the magnetotelluric model, operator
Z
can be written in the form of an
integro-differential transformation. The kernel
G
of the operator by virtue of
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