Methodological guide demonstrates data acquisition and error reduction strategies for single-dish far-infrared polarimetry, highlighting frameworks to interpret interstellar magnetic fields.
We present an introduction to observing procedures and principles of analysis used in far‐infrared polarimetry. The observing procedures are those for single‐dish observations of thermal emission from aligned dust grains. We discuss techniques for removing backgrounds and for reducing and evaluating errors. The principles of analysis are those required for interpreting polarization maps and polarization spectra in terms of opacity, field structure, and variations in temperature and polarizing efficiency.
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Hildebrand et al. (2000) studied this question.