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Waves in Unmagnetized Plasmas
Let us now investigate the cold-plasma dispersion relation in detail. It is
instructive to first consider the limit in which the equilibrium magnetic
field is zero. In the absence of a magnetic field, there is
no preferred direction, so we can, without loss of generality,
assume that
is directed along the
-axis (i.e.,
).
In the zero magnetic field limit (i.e.,
), the eigenmode equation (5.42) reduces to
 |
(5.68) |
where
 |
(5.69) |
Here, we have neglected
with respect to
.
It is clear from Equation (5.68) that there are two types of waves.
The first possesses
the eigenvector
, and has the dispersion relation
 |
(5.70) |
The second possesses the eigenvector
, and has the dispersion
relation
 |
(5.71) |
Here,
,
, and
are arbitrary non-zero quantities.
The former wave has
parallel to
, and is, thus, a
longitudinal (with respect to the electric field) wave. This wave is known as the plasma wave, and
possesses the fixed frequency
. Now, if
is parallel to
then it follows from Equation (5.5)
that
. In other words, the plasma wave is purely electrostatic
in nature. In fact, the plasma wave is an electrostatic oscillation of the type
discussed in Section 1.4.
Because
is independent of
, the so-called group-velocity (Fitzpatrick 2013),
 |
(5.72) |
associated with a plasma wave,
is zero. As is demonstrated in Section 6.7, the group-velocity is the propagation
velocity of localized wave packets. It is clear that the plasma wave
is not a propagating wave, but instead has the property than an oscillation
set up in one region of the plasma remains localized in that region. It
should be noted, however, that in a ``warm'' plasma (i.e., a plasma with a finite
thermal velocity) the plasma wave acquires a non-zero,
albeit very small, group velocity. (See Section 8.2.)
The latter wave is a transverse wave, with
perpendicular to
. There are two independent linear polarizations of this wave,
which propagate at identical velocities,
just like a vacuum electromagnetic wave. The dispersion relation
(5.71) can be rearranged to give
 |
(5.73) |
showing that this wave is just the conventional electromagnetic wave,
whose vacuum dispersion relation is
, modified by
the presence of the plasma. An important conclusion, which follows
immediately from the previous expression, is that this wave can only propagate if
. Because
is
proportional to the square root of the electron number density, it follows that
electromagnetic radiation of a given frequency can only propagate through
an unmagnetized plasma when the electron number density falls below some critical value.
Next: Low-Frequency Wave Propagation
Up: Waves in Cold Plasmas
Previous: Cutoff and Resonance
Richard Fitzpatrick
2016-01-23