AND

We present 43 GHz polarization images obtained with the Very Long Baseline Array of four blazars (0829]046, 1055]018, 1334[127, and AP Librae), as well as four active galactic nuclei, which served as polarization calibrators (DA 193, OJ 287, 3C 279, and 1611]343). Six of these objects are members of the Nartallo et al. millimeter-wave polarization blazar monitoring sample. We Ðnd no di†erences in the overall millimeter-wave polarization properties of the BL Lacertae objects and quasars in our sample. This is in contrast to previous Ðndings at centimeter wavelengths, in which the inferred magnetic Ðelds of quasars are found to be predominantly aligned with the jet, while perpendicular conÐgurations are found in BL Lac objects. With the exception of 1611]343, a low optical polarization quasar, all of the unre-solved blazar cores in our sample have inferred magnetic Ðeld orientations perpendicular to the inner jet direction. Past nonimaging millimeter-wave polarization monitoring data have shown that these core orientations are stable in three of our sample objects; this may be due to strong, unresolved standing shocks located very close to the base of the jet. We also detect in the jets of blazars a moderate-sized population of polarized components having electric vectors that lie at an oblique angle to the local jet direction. We Ðnd that the observed distribution of electric vector misalignment angles cannot be Ðtte