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In this first paper from forthcoming series of works devoted to radio imageof relativistic jets from active galactic nuclei the role of internal structureof a flow is discussed. We determine the radial profiles of all physical valuesfor reasonable Michel magnetization parameter $\sigma_{\rm M}$ and ambientpressure $P_{\rm ext}$. Maps of Doppler boosting factor $\delta$ and observeddirections of linear polarization of synchrotron emission are also constructed.

On the Radio Image of Relativistic Jets -- I. Internal Structure, Doppler Boosting, and Polarization Maps