Evolution of high-m poloidal Alfvén waves in a dipole magnetic field

Thomas Elsden*, Andrew Wright

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

15 Citations (Scopus)
2 Downloads (Pure)

Abstract

We investigate how initially high-m, poloidal Alfvén waves evolve using a numerical model solving the ideal, cold, linear magnetohydrodynamic (MHD) equations in a 2-D dipole coordinate system. The curved magnetic geometry provides a key difference between the poloidal and toroidal Alfvén frequencies of any one field line. A polarization rotation from poloidal toward toroidal predicted from the Cartesian box model theory still occurs but now with the waves following contours of Alfvén frequency, which moves the Alfvén wave across field lines. The structure of these contours depends on the harmonic mode along the field line and the equilibrium. We find that the amplitude peak of the poloidal mode moves significantly radially outward in time. When the typically observed azimuthal phase motion of such waves is included, hodograms show a polarization rotation from purely poloidal to a mixed poloidal/toroidal polarization at all locations. Such features could be used to help interpret satellite observations of Pc4-5 poloidal ultralow frequency (ULF) waves in Earth's magnetosphere.

Original languageEnglish
Article numbere2020JA028187
JournalJournal of Geophysical Research: Space Physics
Volume125
Issue number8
Early online date19 Aug 2020
DOIs
Publication statusPublished - Aug 2020

Keywords

  • Alfven waves
  • high-m
  • magnetosphere
  • MHD
  • simulation
  • ULF waves

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