Skip to main content
Log in

Interactions of Alfvén-Cyclotron Waves with Ions in the Solar Wind

  • Published:
Space Science Reviews Aims and scope Submit manuscript

Abstract

The results of a study of linear and nonlinear properties of Alfvén-cyclotron waves propagating along a background magnetic field in collisionless plasmas are presented. Kinetic theory and one-dimensional hybrid simulations are used to identify the complete family of growing and damped wave modes and the connection with the spontaneous fluctuations in plasmas. The self-consistent reshaping of initially cold ion velocity distributions, the simultaneous generation of beam protons, and the preferential heating and acceleration of alpha particles are shown to occur by the same mechanism: ion trapping and induced pitch-angle scattering by parametrically driven ion acoustic waves.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to J. A. Araneda.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Araneda, J.A., Astudillo, H. & Marsch, E. Interactions of Alfvén-Cyclotron Waves with Ions in the Solar Wind. Space Sci Rev 172, 361–372 (2012). https://doi.org/10.1007/s11214-011-9773-0

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11214-011-9773-0

Keywords

Navigation