Alfvén Waves in Simulations of Solar Photospheric Vortices

S. Shelyag, P. S. Cally, A. Reid, M. Mathioudakis

Research output: Contribution to journalArticlepeer-review

45 Citations (Scopus)

Abstract

Using advanced numerical magneto-hydrodynamic simulations of the magnetized solar photosphere, including non-gray radiative transport and a non-ideal equation of state, we analyze plasma motions in photospheric magnetic vortices. We demonstrate that apparent vortex-like motions in photospheric magnetic field concentrations do not exhibit "tornado"-like behavior or a "bath-tub" effect. While at each time instance the velocity field lines in the upper layers of the solar photosphere show swirls, the test particles moving with the time-dependent velocity field do not demonstrate such structures. Instead, they move in a wave-like fashion with rapidly changing and oscillating velocity field, determined mainly by magnetic tension in the magnetized intergranular downflows. Using time-distance diagrams, we identify horizontal motions in the magnetic flux tubes as torsional Alfvén perturbations propagating along the nearly vertical magnetic field lines with local Alfvén speed.
Original languageEnglish
JournalThe Astrophysical Journal Letters, Volume 776, Issue 1, article id. L4, 4 pp. (2013).
Volume776
Publication statusPublished - 01 Oct 2013

Keywords

  • magnetohydrodynamics: MHD
  • plasmas
  • Sun: magnetic fields
  • Sun: photosphere

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