I determine the displacement of the Sun from the Galactic plane by interpreting IRAS point-source counts at 12 and 25 μm in the Galactic polar caps using the latest version of the SKY model for the point-source sky (Cohen 1994). A value of z_☉ = 15.5 ± 0.7 pc north of the plane provides the best match to the ensemble of useful IRAS data. Shallow K counts in the north Galactic pole are also best fitted by this offset, while limited FAUST far-ultraviolet counts at 1660 A near the same pole favor a value near 14 pc. Combining the many IRAS determinations with the few FAUST values suggests that a value of z_☉ = 15.0 ± 0.5 pc (internal error only) would satisfy these high-latitude sets of data in both wavelength regimes, within the context of the SKY model.
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