Geoscience Reference
In-Depth Information
In order to eliminate the nonzero parallel current
k
E
k
from Eqs. (
6.61
)
and (
6.63
) one should slightly rearrange these equations. Equation (
6.61
) multiplied
by sin plus equation (
6.63
) multiplied by cos gives
@
y
ıB
z
@
z
ıB
y
sin
C
@
x
ıB
y
@
y
ıB
x
cos
D
0
J
?
C
J
.
w
x
sin
C
J
.
w
/
cos
:
z
(6.68)
In the frequency range f<0:1Hz the thickness, l,oftheE layer is much
smaller than the skin-depth in the ionosphere. In this notation the “thin” layer
approximation can be used in order to derive the boundary conditions at the E
layer of the ionosphere. This approximation is described in more detail in Sect. 5.
Integrating of Eq. (
6.68
) with respect to
z
across the E-layer, making formally
l
!
0, and taking into account Eq. (
6.67
), gives the boundary conditions at
z
D
0
sin
ıB
y
D
0
†
P
E
x
= sin
C
†
H
E
y
C
I
.
w
/
;
(6.69)
where the square brackets denote the jump of magnetic field across the E-layer,
†
P
and †
H
are the height-integrated Pedersen and Hall conductivities given by
Eq. (
5.25
). Here I
.
w
/
D
I
.
w
/
x
sin
C
I
.
w
/
z
cos stands for the height-integrated wind-
driven currents, i.e.
Z
Z
l
l
I
.
w
x
D
J
.
w
x
d
z
and I
.
w
z
D
J
.
w
/
z
d
z
:
(6.70)
0
0
Similarly, integrating of Eq. (
6.62
) with respect to
z
across the E-layer yields
ŒıB
x
D
0
†
P
E
y
†
H
E
x
= sin
C
I
.
w
y
;
(6.71)
where I
.
w
/
y
is another component of the height-integrated wind-driven current, i.e.
Z
l
I
.
w
y
D
J
.
w
y
d
z
:
(6.72)
0
In the framework of our model the region above the E-layer is supposed to be
the area consisting solely of a cold collisionless plasma, which is described by
Eq. (
5.2
). In the ULF frequency range the absolute value of parallel components
of the plasma dielectric permittivity, "
k
, is much greater than perpendicular ones
and thus can be assumed to be infinite. This means that the parallel electric field
E
k
equals approximately zero, and we come to Eq. (
6.67
). Thus, we can eliminate the
parallel current from Eq. (
5.2
) in analogy to the procedure used for the derivation of
Eq. (
6.68
). Whence, we get
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