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decrement with the number beginning with the resonance period of about
20 s.
Consider the dependence of the decrement on Pedersen conductivity. At
large
Σ
P
(dayside ionosphere), when
Σ
P
=4
πΣ
P
c
A
/c
2
1, the decrement
Σ
P
γ
1
∝
1
/Σ
P
vanishes (
Σ
P
→∞
). At
1 when the
Σ
P
is small (night
Σ
P
.At
Σ
P
→
ionosphere), the decrement
γ
1
∝
1, the coecient of reflection
of the Alfven wave vanishes and
γ
1
→∞
. This effect is connected with the
'thin' ionosphere approximation and for the 'thick' ionosphere
γ
is finite.
Resonance Electric and Magnetic Fields Along a Field-Line
Distribution of the electric and magnetic wave components along a resonance
field line is determined by
e
j
(
x
) (6.79). In the dipole magnetic field the physical
components of the azimuthal magnetic field
b
ϕ
and orthogonal to the magnetic
shells electric field
E
ν
are determined by (6.89), (6.90). Keeping only the main
terms in (6.89), (6.90), we obtain the distribution of
b
ϕ
and
E
ν
along the field
line at the shell
ν
=
ν
r
:
b
ϕ
≈
x
2
)
−
3
/
2
e
(
j
1
(
x
)
,
ν
r
(1
−
E
ν
≈
x
2
)
−
3
/
2
(1 + 3
x
2
)
1
/
2
e
(
j
2
(
x
)
,
ν
r
(1
−
(6.124)
where
x
=cos
θ
is the coordinate of a point on a field-line.
An example of the distribution of the FLR-fields for two harmonics along
a field line
L
= 2 is shown in Fig. 6.8. Figures 6.8a and 6.8b represent,
respectively, the fields of the 2-nd harmonic with resonance frequency
ω
2
=
0
.
6136
0
.
1323
i
. One can
see that ionospheric fields are larger than magnetospheric ones. The amplitude
of the magnetic field decreases steeply in the ionospheric
F
-layer. The electric
−
0
.
1186
i
and the 3-rd harmonics with
ω
3
=0
.
6336
−
1
1
2
10
10
2
0
0
4
−10
−10
3
4
3
−20
−20
−30
a
−30
b
−40
−40
−50
−50
0
0.2
0.4
0.6
0.8
0
0.2
0.4
0.6
0.8
cos θ
cos θ
Fig. 6.8.
Field line distribution of the electric (
e
2
) and magnetic (
e
1
) wave com-
ponents at
L
=2
.
a) the 2-nd FLR-harmonics with the resonance frequency
ω
2
=0
.
6136
−
0
.
1186
i
;(b)the3-rdharmonics
ω
3
=0
.
6336
−
0
.
1323
i.
Indexes 1
and 3 refer, respectively, to real parts of
e
1
and
e
2
and 2
,
4 - to their imaginary
parts. The azimuthal magnetic component
b
ϕ
and the electric component orthogo-
nal to the
E
ν
magnetic shell are connected with
e
1
and
e
2
by (6.124)
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