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A method of accelerated computation of broadband far-off boresight patterns of telescope beams is extended and applied to the 100 GHz channels of Planck HFI (HFI – 100). Far-off boresight angle power patterns are computed with both GRASP-PTD and NUIM-PO software, considering cuts with an angular size of 10 degrees. The former reveal secondary oscillations of radial power distribution as compared with the latter. The difference for power patterns of a/b polarisation channels is also investigated.

PTD vs PO effects in power and polarization of Planck HFI-100 beams