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 Alfvén 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. Copyright 2003 by the American Geophysical Union.
CITATION STYLE
Galsgaard, K., Priest, E. R., & Titov, V. S. (2003). Numerical experiments on wave propagation toward a 3D null point due to rotational motions. Journal of Geophysical Research: Space Physics, 108(A1). https://doi.org/10.1029/2002JA009393
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