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can get aligned by radiative torque and the aligned grains can produce polarized emission in infrared wavelengths. We explore alignment of dust grains by radiative torque in T Tauri disks and provide predictions for polarized emission for disks viewed at different wavelengths and viewing angles. Our study indicates
that multi-frequency infrared polarimetric studies of protostellar disks can provide good insights into the details of their magnetic structure. We also introduce the result and implications of a more recent observation at 350 microns.