Diverse Polarimetric Features of AGN Jets from Various Viewing Angles: Towards a Unified View

Here, we demonstrate that polarization properties show a wide diversity depending on viewing angles. To simulate images of supermassive black hole and surrounding plasma, performed full-polarimetric general relativistic radiative transfer based three-dimensional magnetohydrodynamics models with moderate magnetic strengths. Under an assumption hot-jet cold-disk in the electron temperature prescription, confirmed typical scenario where polarized synchrotron emissions from funnel jet experience Faraday rotation conversion equatorial disk. Further, found linear vectors are inevitably depolarized for edge-on-like observers, whereas portion survive reach observers face-on-like cases. We also circular components have persistent signs face-on cases, changing edge-on It is these features smoothly connected via intermediate viewing-angle These results due to rotation/conversion different angles, suggest combination polarimetry can give constraint inclination between observer hole's (and/or disk's) rotating-axis plasma jet--disk structure. lead more statistical unified interpretation active galactic nuclei.