Propagating Alfvén waves in open structures with random structuring

D. J. Pascoe*, I. De Moortel, P. Pagano, T. A. Howson

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)
55 Downloads (Pure)

Abstract

We consider the behaviour of Alfvén waves propagating in a medium with random density perturbations. The imposed density perturbations have a broad-band spectrum and their characteristic spatial scale may be defined according to the peak in the spectrum. The interaction of the boundary driven Alfvén waves with the medium generates reflections most efficiently when their wavelength is comparable to the spatial scale of the density perturbations. For our monotonic driver, this leads to the generation of quasi-periodic oscillations. The periods of oscillation of the propagating Alfvén waves is no longer only associated with the driver. Additional periodicities may be associated with one or more characteristic spatial scales in the density profile, or with beating between other spectral components. Multiple wave reflections cause oscillatory power to be retained at low altitudes, increasing opportunities to contribute to heating at those locations.

Original languageEnglish
Pages (from-to)2181-2188
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume516
Issue number2
Early online date23 Aug 2022
DOIs
Publication statusPublished - 1 Oct 2022
Externally publishedYes

Keywords

  • MHD
  • Sun: atmosphere
  • Sun: corona
  • Sun: oscillations

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