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Lazarian, Diego F. Gonz\\'alez-Casanova","submitted_at":"2016-08-24T15:40:55Z","abstract_excerpt":"Strong Alfv\\'enic turbulence develops eddy-like motions perpendicular to the local direction of magnetic fields. This local alignment induces velocity gradients perpendicular to the local direction of the magnetic field. We use this fact to propose a new technique of studying the direction of magnetic fields from observations, the Velocity Gradient Technique. We test our idea by employing the synthetic observations obtained via 3D MHD numerical simulations for different sonic and Alfv\\'en Mach numbers. We calculate the velocity gradient, $\\mathbf{\\Omega}$, using the velocity centroids. 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