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Paper: Hertz and SCUBA: Submillimeter Polarimetry of Molecular Clouds from Mauna Kea
Volume: 449, Astronomical Polarimetry 2008: Science from Small to Large Telescopes
Page: 163
Authors: Vaillancourt, J. E.; Matthews, B. C.
Abstract: Polarization maps of Galactic clouds at multiple far-infrared and submillimeter wavelengths have been used to study changing magnetic field structure with cloud depth, as well as put limits on dust grain shape, temperature, emissivity, and alignment efficiency. To date, few detailed studies have been carried out on individual clouds at multiple wavelengths. We identify 15 clouds which have been mapped in polarization at both 350 and 850 μm and compare the polarization amplitudes and position angles at the two wavelengths. This more than triples the number of clouds at which direct comparisons have been made at 350 and 850 μm.
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