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A strongly nonlinear Alfvénic pulse in a transversely inhomogeneous medium

  • D. Tsiklauri
  • , V. M. Nakariakov
  • , T. D. Arber

Research output: Contribution to journalArticlepeer-review

38 Citations (Scopus)

Abstract

We investigate the interaction of a plane, linearly polarized, Alfvénic pulse with a one-dimensional, perpendicular to the magnetic field, plasma density inhomogeneity in the strongly nonlinear regime. Our numerical study of the full MHD equations shows that: (i) Plasma density inhomogeneity substantially enhances (by about a factor of 2) the generation of longitudinal compressive waves. (ii) Attained maximal values of the generated transverse compressive perturbations are insensitive to the strength of the plasma density inhomogeneity, plasma β and the initial amplitude of the Alfvén wave. Typically, they reach about 40% of the initial Alfvén wave amplitude. (iii) Attained maximal values of the generated relative density perturbations are within 20-40% for 0.5 ≤ β ≤ 2.0. They depend upon plasma β strongly; and scale almost linearly with the initial Alfvén wave amplitude.

Original languageEnglish
Pages (from-to)285-292
Number of pages8
JournalAstronomy and Astrophysics
Volume395
Issue number1
DOIs
Publication statusPublished - Nov 2002

Keywords

  • Magnetohydrodynamics (MHD)
  • Sun: activity
  • Sun: solar wind
  • Waves

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