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6.6 Summary
In this chapter we treated both free and excited oscillations and the structure
of the MHD-waves in the axially symmetric magnetospheric models as well.
1. We found that spectrums of Alfven oscillations in 2D case can be reduced
to two 1D boundary problems:
determination of the toroidal oscillation spectrum from (6.51), (6.53)
and
determination of the poloidal oscillation spectrum from (6.52), (6.54).
2. We examined also the excitement of the oscillations by a harmonic source
of frequency ω close to the frequency ω ( T j ( L r ) of the toroidal resonance
mode j of one of the FLR-shells with L = L r . It was shown that the spatial
distribution of the azimuthal magnetic component b ϕ and of the electric
component E ν orthogonal to the FLR-shellin the toroidal mode are Lorentz
resonance curves:
b ( j )
E ( j )
ϕ
ϕ
b ϕ
E ν
,
,
( L r + ( j L )
( L r + ( j L )
L
L
ϕ and E ( j ) ν can be found from the longitudinal magnetic compo-
nent b (see (6.113), (6.114)).
3. The decrement γ ( T )
j
where b ( j )
( L ) of the toroidal oscillations is connected with the
half-width δ ( j )
L
and the spatial scale of the FLR-frequency ω ( T )
j
:
d ω ( T )
j
d L
1
δ ( j )
L
γ ( T )
j
.
L = L r
4. Besides of toroidal modes, there are also poloidal modes. Contrary to
toroidal oscillations which manifest themselves in azimuthal magnetic com-
ponents and in electrical components orthogonal to the shell, poloidal os-
cillations of the shell are resonance oscillations of the magnetic component
orthogonal to the shell and of the azimuthal electric component.
5. Polarization splitting of the FLR-frequencies for the toroidal and poloidal
oscillations is determined by the difference of the two main curvatures of
the surface orthogonal to geomagnetic field-lines. In other words, the split
is determined by the difference of the convergency / divergency rate of the
field-lines within the meridional and equatorial plains.
Appendix A
The metric tensors g ik and g ik
of the non-orthogonal system coordinates
x 1 ,x 2 ,x 3
{
}
are
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