Numerical experiments on wave propagation towards a 3D null point due to rotational motions

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Abstract

[1] We describe 3D resistive magnetohydrodynamic (MHD) numerical experiments at a null point driven by the rotation of magnetic field lines near the spine of the null. When field lines around the spine are rotated, a twist wave propagates toward the null along field lines, satisfying a Klein - Gordon equation. While the helical Alfven wave spreads out as the null is approached, a fast-mode wave focuses on the null and wraps around it. Only a weak diffusion of the twisted field line structure is found to take place.

Original languageEnglish
Article number1042
Number of pages9
JournalJournal of Geophysical Research
Volume108
Issue numberA1
DOIs
Publication statusPublished - 28 Jan 2003

Keywords

  • 3-DIMENSIONAL MAGNETIC RECONNECTION
  • STEADY-STATE
  • SOLAR CORONA
  • FLUX TUBES
  • TURBULENCE
  • DYNAMICS
  • HELICITY
  • FIELDS
  • MODEL
  • FLOWS

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