Model of the polarized foreground diffuse Galactic emissions from 33 to 353Â GHz

► We present 3D models of the Galactic magnetic field including regular and turbulent components. ► We compute the expected dust and synchrotron emission. ► We compare expectations to the WMAP and Archeops data. ► We propose a consistent model of the Galaxy in the frequency range from 33 to 353 GHz. ► Model useful for CMB studies.