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Home/Electricity & Magnetism/Radiation Belts Drift Shells

Radiation Belts Drift Shells

Earth’s radiation belts trap energetic charged particles on dipole magnetic field lines. In the adiabatic (guiding-center) picture, the first invariant μ = mv⊥²/(2B) is conserved, so a particle’s equatorial pitch angle α sets where it mirrors as B grows along the line. Particles with α below the equatorial loss cone α_lc strike the atmosphere and are lost; larger α are stably trapped on an L-shell (equatorial crossing radius r = L R_E in the dipole approximation). Superimposed on rapid gyration and bounce motion is a slow azimuthal drift from magnetic field gradients and line curvature: in a dipole, protons drift eastward and electrons westward around Earth. The teaching model uses a centered dipole B-field, equatorial drift speed v_d ∝ K L² (with relativistic γ at high energy), animated motion on a circular L-shell in the top view, a meridional slice showing the field line, mirror point, pitch angle, and loss-cone wedge, and a plot of α_lc versus L from footpoints at ~100 km altitude. It does not include wave diffusion, realistic magnetosphere asymmetry, or slot-region dynamics.

Who it's for: Space physics or upper-level E&M students after dipole fields and before ring-current or wave-particle interaction modules.

Key terms

  • Van Allen radiation belts
  • L-shell
  • Gradient drift
  • Curvature drift
  • Loss cone
  • Pitch angle
  • Magnetic mirror

Radiation belts

3
500keV
45°
1×

Van Allen belt drift shells: charged particles gradient- and curvature-drift around Earth on dipole L-shells. Equatorial pitch angle α sets mirror latitude; particles with α < α_lc are in the atmospheric loss cone.

Measured values

Drift speed v_d42.91km/s
Drift period T_d46.6 min
Loss cone α_lc8.6°
StatusTrapped

How it works

Van Allen radiation belts: gradient and curvature drift on dipole L-shells, mirror points, and equatorial loss cone — electrons west, protons east.

Frequently asked questions

Why do electrons and protons drift opposite ways?
Gradient and curvature drifts depend on charge sign. In Earth’s dipole, protons drift east and electrons west around the planet.
What is the loss cone?
At the equator, particles with pitch angles below α_lc have mirror points below the atmosphere and precipitate; larger angles are trapped.
What is an L-shell?
In the dipole approximation, L is the equatorial crossing distance in Earth radii: r_eq = L R_E. Constant-μ drift orbits follow L-shells at low pitch angles.
What is omitted?
Offset dipole, local time asymmetry, radial diffusion, plasmasphere, and electromagnetic wave scattering are not modeled.