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A great deal can be learnt about the energetization of particles
around the Earth, particularly in the production of very fast (1000
km/s) particles, by using individually particle tracking algorithms,
with the electric and magnetic fields provided by the gloabl modeling
seen on the other pages. A few examples are shown below, where the
particles velocities are color coded - grey/ blue relatively slow at
50-100 km/s, green at ~ 300 km/s and red at > 1000 km/s.
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A
movie (2.3 Mbyte)showing the deflection and
energization of solar wind
particles at
Earth.
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A movie
(1.0 Mbyte) showing the loss of ionospheric particles from the northern hemisphere, and the formation of
energetic particles rings around the Earth. |
| An
important way to monitor space conditions is to sample the particle
populations as they move along the terrestrial magnetic field
and reach
low atitudes. Here is a movie (8 Mbytes) of the mapping
of these particles onto the northern hemisphere. |