Fig. 6.
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Alfvén identifier νA for numerical data (left) and the MUSE synthetic emission (right) at t = 193 s. For the synthetic emission, 
, where vy is the Doppler velocity observed from the direction parallel to the loop (y-LOS). For the numerical simulation, νA = (∇ × v)⋅B/B (i.e. it includes derivatives and magnetic field in all directions) at y = 0 Mm.
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