Magnetized interstellar turbulence simulations generate synthetic dust polarization maps that reproduce Planck E- and B-mode spectral properties at 353 GHz while explaining observed E/B asymmetry and positive TE signal.
Koley,Publ
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$Ab$ $initio$ modeling of Galactic dust polarized CMB foreground
Magnetized interstellar turbulence simulations generate synthetic dust polarization maps that reproduce Planck E- and B-mode spectral properties at 353 GHz while explaining observed E/B asymmetry and positive TE signal.