Formation, Propagation, and Decay of Coherent Pulses of Solar Cosmic Rays

Details Formation, Propagation, and Decay of Coherent Pulses of Solar Cosmic Rays Formation, Propagation, and Decay of Coherent Pulses of Solar Cosmic Rays

1995-06-28

arxiv.org/abs/astro-ph/9506133v1

Geophys. Res. Lett. 22 (1995) 2073

Astronomy and Astrophysics

Astrophysics

4 pages (LaTeX) + 4 uuencoded-tarred-compressed postscript figures, uses agupp.sty (available from ftp://xxx.lanl.gov/macros o

Scientific paper

We have performed numerical simulations of the interplanetary transport of solar cosmic rays. The particles form a coherent pulse within $\sim0.01$ AU after their injection. The gradual decrease of a pulse's speed and anisotropy can be understood in terms of an equilibrium between pitch-angle scattering and focusing. The results should be useful for estimating times of particle injection.

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