Geoscience Reference
In-Depth Information
the field-lines as well as the 2D or 3D inhomogeneity of the plasma are taken
into account is performed in Chapter 6.
Suppose that the magnetic field
B
0
=
B
0
z
. Then, if no external forces are
acting on the plasma, the pressure is
P
0
=
P
0
(
x, y
) and the magnetic field is
B
0
=
B
0
(
x, y
) . Using the vector equality
B
0
]=
B
0
∂
ξ
⊥
∂z
−
∇
×
[
ξ
⊥
×
z
[
B
0
∇
·
ξ
⊥
+(
ξ
⊥
·
∇
⊥
)
B
0
]
we reduce (4.21) to
ρ
0
c
2
A
∇
⊥
ρ
0
c
2
A
+
c
s
∇·
1
L
ξ
⊥
=
−
ξ
⊥
c
s
∇
⊥
ρ
0
+
+
ρ
0
c
s
,
∂
ξ
ρ
0
c
2
A
2
∂z
+
ξ
⊥
·
∇
⊥
(4.22)
c
s
,
ρ
0
c
2
A
2
1
ρ
0
c
s
∂
∂z
L
s
ξ
=
−
∇
·
(
ρ
0
ξ
⊥
)+
ξ
⊥
·
∇
⊥
(4.23)
where
c
2
A
=
B
0
/
4
πρ
0
is the Alfven velocity,
∂
2
∂z
2
−
∂
2
∂t
2
,
1
c
2
A
L
=
∂
2
∂z
2
−
∂
2
∂t
2
.
1
c
s
L
s
=
4.2 Homogeneous Plasma
Basic Equations
Propagation of small-amplitude hydromagnetic waves in homogeneous plasma
is discussed in most textbooks on plasma physics and magnetohydrodynamics
([5], [6], [15], [18]), and even more so in works specially devoted to electro-
magnetic wave propagation in plasma ([9], [19]). The basic properties of these
waves are briefly described in this section. Hydromagnetic waves in the ho-
mogeneous case will be analyzed in a way convenient for generalization on
inhomogeneous media.
In a homogeneous medium
∇
ρ
0
,
∇
c
A
,
and
∇
c
s
vanish and (4.22) - (4.23)
reduce to
(1 +
β
)
,
ξ
⊥
+
β
∂
ξ
||
∂z
L
ξ
⊥
=
−
∇
⊥
∇
·
(4.24)
∂
∂z
∇
·
L
s
ξ
||
=
−
ξ
⊥
,
(4.25)
where
β
=
c
s
/c
2
A
.
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