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We present numerical relativistic magnetohydrodynamic and emissionsimulations aimed to study the role played by the magnetic field in thedynamics and emission of relativistic jets in Active Galactic Nuclei. We focusour analysis on the study of the emission from recollimation shocks since theymay provide an interpretation for the stationary components seen atparsec-scales in multiple sources. We show that the relative brightness of theknots associated with the recollimation shocks decreases with increasing jetmagnetization, suggesting that jets presenting stationary components may have arelatively weak magnetization, with magnetic fields of the order ofequipartition or below.

The Influence of Helical Magnetic Fields in the Dynamics and Emission of Relativistic Jets