Effect of proton-amplified waves on the evolution of solar energetic particle composition in gradual events

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Solar Physics, Astrophysics, And Astronomy: Energetic Particles, Interplanetary Physics: Interplanetary Shocks, And Astronomy: Coronal Mass Ejections, Interplanetary Physics: Plasma Waves And Turbulence

Scientific paper

We present a model of the coupled evolution of energetic ions and Alfvén waves, incorporating magnetic focusing, pitch-angle diffusion, wave amplification, and a traveling ion source. Ion transport through protonamplified waves with non-Kolmogorov spectra produces the contrasting three-stage evolution of Fe/O and He/H ratios at several MeV/amu observed by Wind/EPACT in the 20 April 1998 gradual solar energetic particle event [Tylka et al., 1999].

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