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Heavy Ion Acceleration by Super-Alfvenic Waves

Space Physics 2020-01-09 v1 High Energy Astrophysical Phenomena Solar and Stellar Astrophysics

Abstract

A generation mechanism of super Alfv\'{e}nic (SPA) waves in multi-ion species plasma is proposed and the associated heavy ion acceleration process is discussed. The SPA waves are thought to play important roles in particle acceleration since they have large wave electric field because of their high phase velocity. It is demonstrated by using full particle-in-cell simulation that large amplitude proton cyclotron waves, excited due to proton temperature anisotropy, nonlinearly destabilize SPA waves through parametric decay instability in a three component plasma composed of electrons, protons, and α\alpha particles. At the same time, α\alpha cyclotron waves get excited via another decay instability. A pre-accelerated α\alpha particle resonates simultaneously with the two daughter waves, the SPA waves and the α\alpha cyclotron waves, and it is further accelerated perpendicular to the ambient magnetic field. The process may work in astrophysical environments where sufficiently large temperature anisotropy of lower mass ions occurs.

Keywords

Cite

@article{arxiv.2001.02538,
  title  = {Heavy Ion Acceleration by Super-Alfvenic Waves},
  author = {S. Matsukiyo and T. Akamizu and T. Hada},
  journal= {arXiv preprint arXiv:2001.02538},
  year   = {2020}
}

Comments

4 figures

R2 v1 2026-06-23T13:05:59.417Z