Geoscience Reference
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Fig. 1.16 Thesamefield
components as shown in
Fig. 1.15 but for fast and slow
magnetosonic (FMS and
SMS) waves
z
E
y
ʴ B
V
ʸ
B 0
k
x
Substituting Eq. ( 1.62 )forı B into Eq. ( 1.63 ), taking into account the vector identity
( 1.55 ), and rearranging we arrive at
! 2
k 2 V A V D c s . k V / k k 2 . V V A / V A ;
(1.64)
where V A and V A are given by Eqs. ( 1.60 ) and ( 1.61 ). Projections of this vector
equation onto x and y axes can be written as
a xx V x C a xy V y D 0;
(1.65)
a yx V x C a yy V y D 0;
(1.66)
where the matrix coefficients are given by
a xx;yy D ! 2
k 2 V A c s k x;y C k 2 V Ax;y ;
(1.67)
a xy D a yx D k 2 V Ax V Ay c s k x k y ;
(1.68)
and V Ax and V Ay denotes the projections of the vector V A onto the coordinate axes
x and y.
The set of Eqs. ( 1.65 )-( 1.66 ) has a nontrivial solution for V x and V y only if the
determinant of the set is equal to zero. Hence we come to the following dispersion
relation
n V A C c s ˙
h V A C c s 2
4c s . O x V A / 2 io 1=2
! 2
k 2 D
1
2
;
(1.69)
where O x stands for the unit vector parallel to k . This equation describes two different
modes. The sign plus in Eq. ( 1.69 ) determines the mode, which is referred to as the
fast magnetosonic (FMS) wave while the sign minus corresponds to the so-called
slow magnetosonic (SMS) wave. Below we show that the fast wave propagates
almost isotropically, while the slow wave is a strongly anisotropic mode. Both the
magnetosonic modes readily carry a field-aligned magnetic perturbation; that is,
they describe a magnetically compressive mode.
 
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