Skip to main content
Log in

Alfvén Wave Phase Mixing as a Source of Fast Magnetosonic Waves

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

The nonlinear excitation of fast magnetosonic waves by phase mixing Alfvén waves in a cold plasma with a smooth inhomogeneity of density across a uniform magnetic field is considered. If initially fast waves are absent from the system, then nonlinearity leads to their excitation by transversal gradients in the Alfvén wave. The efficiency of the nonlinear Alfvén–fast magnetosonic wave coupling is strongly increased by the inhomogeneity of the medium. The fast waves, permanently generated by Alfvén wave phase mixing, are refracted from the region with transversal gradients of the Alfvén speed. This nonlinear process suggests a mechanism of indirect plasma heating by phase mixing through the excitation of obliquely propagating fast 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

Rights and permissions

Reprints and permissions

About this article

Cite this article

Nakariakov, V.M., Roberts, B. & Murawski, K. Alfvén Wave Phase Mixing as a Source of Fast Magnetosonic Waves. Solar Physics 175, 93–105 (1997). https://doi.org/10.1023/A:1004965725929

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1004965725929

Keywords

Navigation