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Three dimensional magnetohydrodynamical simulations were carried out in orderto perform a new polarization study of the radio emission of the supernovaremnant SN 1006. These simulations consider that the remnant expands into aturbulent interstellar medium (including both magnetic field and densityperturbations). Based on the referenced-polar angle technique, a statisticalstudy was done on observational and numerical magnetic field position-angledistributions. Our results show that a turbulent medium with an adiabatic indexof 1.3 can reproduce the polarization properties of the SN 1006 remnant. Thisstatistical study reveals itself as a useful tool for obtaining the orientationof the ambient magnetic field, previous to be swept up by the main supernovaremnant shock.

A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case