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 3 shows the Dst index for the month of March 1989.The 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.
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, 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
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.