D. Ruffolo et T. Khumlumlert, FORMATION, PROPAGATION, AND DECAY OF COHERENT PULSES OF SOLAR COSMIC-RAYS, Geophysical research letters, 22(15), 1995, pp. 2073-2076
We have performed numerical simulations of the interplanetary transpor
t of solar cosmic rays. The particles form a coherent pulse within sim
ilar to 0.01 AU after their injection. The gradual decrease of a pulse
's speed and anisotropy can be understood in terms of an equilibrium b
etween pitch-angle scattering and focusing. The results should be usef
ul for estimating times of particle injection.