Fig. 17

Maps of a few selected regions illustrating the relation between polarization
fraction and polarization angle dispersion function. Rows from top to bottom
show total intensity at 353
GHz, polarized intensity, polarization fraction, and polarization
angle dispersion function, .
Columns from left to right are for Taurus, Orion, Ophiuchus, and
Polaris. The polarization segments show the orientation of the apparent magnetic
field, but their length is constant, not reflecting the changing polarization
fraction. Note that the boundaries of the regions shown here do not match exactly
those in Table 1 and Fig. 6.
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