摘要： We present 11.1 to 37.1 μm imaging observations of the very dense molecular cloud core MM1 in G034.43+00.24 using FORCAST on SOFIA and submillimeter (submm) polarimetry using SHARP on the Caltech Submillimeter Observatory. We ?nd that at the spatial resolution of SOFIA, the point-spread function (PSF) of MM1 is consistent with being a single source, as expected based on millimeter (mm) and submm observations. The spectral energy distributions (SEDs) of MM1 and MM2 have a warm component at the shorter wavelengths not seen in mm and submm SEDs. Examination of H(1.65 μm) stellar polarimetry from the Galactic Plane Infrared Polarization Survey shows that G034 is embedded in an external magnetic ?eld aligned with the Galactic Plane. The SHARP polarimetry at 450 μm shows a magnetic ?eld geometry in the vicinity of MM1 that does not line up with either the Galactic Plane or the mean ?eld direction inferred from the CARMA interferometric polarization map of the central cloud core, but is perpendicular to the long ?lament in which G034 is embedded. The CARMA polarimetry does show evidence for grain alignment in the central region of the cloud core, and thus does trace the magnetic ?eld geometry near the embedded Class 0 YSO.