Ck. Ng et al., Effect of proton-amplified waves on the evolution of solar energetic particle composition in gradual events, GEOPHYS R L, 26(14), 1999, pp. 2145-2148
We present a model of the coupled evolution of energetic ions and Alfven wa
ves, incorporating magnetic focusing, pitch-angle diffusion, wave amplifica
tion, and a traveling ion source. Ion transport through proton-amplified wa
ves with non-Kolmogorov spectra produces the contrasting three-stage evolut
ion of Fe/O and He/H ratios at several MeV/amu observed by Wind/EPACT in th
e 20 April 1998 gradual solar energetic particle event [Tylka et al., 1999]
.