Abstract
We have performed numerical simulations of the interplanetary transport of solar cosmic rays. The particles form a coherent pulse within ∼0.01 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.
| Original language | English |
|---|---|
| Pages (from-to) | 2073-2076 |
| Number of pages | 4 |
| Journal | Geophysical Research Letters |
| Volume | 22 |
| Issue number | 15 |
| DOIs | |
| Publication status | Published - 1 Aug 1995 |
| Externally published | Yes |
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