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Up: Charged particle motion
Previous: The Van Allen radiation
Up to now, we have only considered the lowest order motion (i.e.,
gyration combined with parallel drift) of charged particles in the
magnetosphere. Let us now examine the higher order corrections to this
motion. For the case of non-time-varying fields, and a weak electric
field, these corrections consist of a combination of
drift,
grad-
drift, and curvature drift:
 |
(138) |
Let us neglect
drift, since this motion merely gives
rise to the convection of plasma within the magnetosphere, without generating a
current. By contrast, there is a net current associated with grad-
drift
and curvature drift. In the limit in which this current does not strongly
modify the ambient magnetic field (i.e.,
),
which is certainly the situation in the Earth's magnetosphere, we can write
 |
(139) |
It follows that the higher order drifts can be combined to give
 |
(140) |
For the dipole field (121), the above expression yields
 |
(141) |
Note that the drift is in the azimuthal direction. A positive drift velocity
corresponds
to eastward motion, whereas a negative velocity corresponds to westward motion.
It is clear that, in addition to their gyromotion and periodic
bouncing motion along field-lines, charged particles trapped
in the magnetosphere also
slowly precess around the Earth. The ions drift westwards and the electrons
drift eastwards, giving rise to a net westward current circulating around the
Earth. This current is known as the ring current.
A typical trajectory of a charged particle, including the bounce motion and
precessional drift, but excluding the gyromotion for the sake of clarity, is
shown in Fig. 4.
Figure 4:
Typical trajectory of a charged particle in the Earth's
magnetosphere, excluding gyromotion.
 |
Although the perturbations to the Earth's magnetic field induced by the ring
current are small, they are still detectable. In fact, the ring current
causes a slight reduction in the Earth's magnetic field in equatorial
regions. The size of this reduction is a good measure of the
number of charged particles contained in the Van Allen belts. During
the development of so-called geomagnetic storms, charged particles are
injected into the Van Allen belts from the outer magnetosphere, giving rise
to a sharp increase in the ring current, and a corresponding decrease in the
Earth's equatorial magnetic field. These particles eventually precipitate
out of the magnetosphere into the upper atmosphere
at high latitudes, giving rise to intense
auroral activity, serious interference in electromagnetic communications, and, in extreme
cases, disruption of electric
power grids. The ring current induced reduction in the
Earth's magnetic field is measured by the so-called
Dst index, which is based on
hourly averages of the northward horizontal component of the terrestrial
magnetic
field recorded at four low-latitude observatories; Honolulu (Hawaii),
San Juan (Puerto Rico), Hermanus (South Africa),
and Kakioka (Japan). Figure 5 shows the Dst index for the month of March
1989.6The very marked reduction in the index, centred about March 13th, corresponds
to one of the most severe geomagnetic storms experienced in recent decades.
In fact, this particular storm was so severe that it tripped out the
whole Hydro Quebec electric distribution system, plunging more than 6 million
customers into darkness. Most of Hydro Quebec's neighbouring systems in the United
States came uncomfortably close to experiencing the same cascading power
outage scenario. Note that a reduction in the Dst index by 600nT
corresponds to a
reduction in the terrestrial magnetic field at the equator.
Figure 5:
Dst data for March 1989 showing an exceptionally
severe geomagnetic storm on the 13th.
 |
According to Eq. (141), the precessional drift velocity of charged particles
in the magnetosphere is a rapidly decreasing function of increasing latitude
(i.e., most of the ring current is concentrated in the equatorial plane).
Since particles typically complete many bounce orbits during a full rotation around
the Earth (see Fig. 4), it is convenient to average Eq. (141) over a bounce
period to obtain the average drift velocity. This averaging can
only be performed numerically. The final answer is well approximated by
 |
(142) |
The average drift period (i.e., the time required to
perform a complete rotation around the Earth) is simply
 |
(143) |
Thus, the drift period for protons and electrons is
 |
(144) |
Note that MeV energy electrons and ions precess around the Earth with about the same
velocity, only in opposite directions, because there is no explicit
mass dependence in Eq. (142). It typically takes an hour to perform a full
rotation.
The drift period only depends weakly on
the equatorial pitch angle, as is the case for the bounce period.
Somewhat paradoxically, the drift period is
shorter on more distant
-shells.
Note, of course, that particles only get a chance to complete a
full rotation around the Earth if the inner magnetosphere remains quiescent
on time-scales of order an hour, which is, by no means, always the case.
Note, finally, that, since the rest mass of an electron is
MeV, most
of the above formulae require relativistic correction when applied to
MeV energy electrons.
Fortunately, however, there is no such problem for protons, whose rest mass
energy is
GeV.
Next: The second adiabatic invariant
Up: Charged particle motion
Previous: The Van Allen radiation
Richard Fitzpatrick
2006-02-16