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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.
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Galsgaard et al. (2003) studied this question.
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