Alfvén Wave Phase Mixing as a Source of Fast Magnetosonic Waves

VM Nakariakov, Bernard Roberts, K Murawski

Research output: Contribution to journalArticlepeer-review

136 Citations (Scopus)

Abstract

The nonlinear excitation of fast magnetosonic waves by phase mixing Alfven 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 Alfven wave. The efficiency of the nonlinear Alfven-fast magnetosonic wave coupling is strongly increased by the inhomogeneity of the medium. The fast waves, permanently generated by Alfven wave phase mixing, are refracted from the region with transversal gradients of the Alfven speed. This nonlinear process suggests a mechanism of indirect plasma heating by phase mixing through the excitation of obliquely propagating fast waves.

Original languageEnglish
Pages (from-to)p.93-105.
Number of pages13
JournalSolar Physics
Volume175
Issue number1
Publication statusPublished - Sept 1997

Keywords

  • FLUX-CORRECTED TRANSPORT
  • CORONAL HEATING MECHANISMS
  • SOLAR CORONA
  • PLASMA
  • ALGORITHM
  • MODES

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