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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