Magnetic Storm (2D)

Charged particles streaming through a planetary dipole field. Each particle feels the real Lorentz force F = q v × B, with B falling off as the inverse cube of distance from the core — the same law that shapes Earth's magnetosphere.

Particles0
Trapped (mirroring)0%
Core field |B₀|0.00
Mean gyroradius0.00
Drag anywhere to nudge the solar-wind injection direction.