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 language | English |
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Article number | 1042 |
Number of pages | 9 |
Journal | Journal of Geophysical Research |
Volume | 108 |
Issue number | A1 |
DOIs | |
Publication status | Published - 28 Jan 2003 |
Keywords
- 3-DIMENSIONAL MAGNETIC RECONNECTION
- STEADY-STATE
- SOLAR CORONA
- FLUX TUBES
- TURBULENCE
- DYNAMICS
- HELICITY
- FIELDS
- MODEL
- FLOWS