Passing particles in toroidal geometry are described in a Hamiltonian
formalism including time-dependent electric and magnetic fields. These
particles are characterized by a non-vanishing toroidal velocity. The
introduction of the toroidal angle as independent variable instead of the
time allows one to derive a map of the poloidal plane onto itself, which is
similar to the Poincaré map of magnetic field lines. In time-dependent
fields the energy of the particles is not conserved leading to two coupled
maps, which is characteristic for autonomous systems with three degrees of
freedom. As a result, Arnold diffusion occurs and Kolmogorov-Arnold-Moser (KAM) surfaces, which in
the case of energy conservation separate stochastic regions in phase space,
can be bypassed leading to enhanced radial transport of particles. The
mechanism of enhanced transport is resonance streaming along resonance
lines, which constructs the complex Arnold web. The structure of this web
depends on the drift rotational transform of drift orbits and the toroidal
transit time of passing particles. Numerical examples of Arnold diffusion
of test particles will be given. The theory will be applied to passing
particles in a toroidal plasma and to trapped particles in stellarators and
tokamaks. Some numerical examples of Arnold diffusion of circulating
particles will be given.