  We present Faraday Rotation Measure (RM) values derived at L- and P-band as
well as some 60 Stokes-parameter profiles, both determined from our
longstanding Arecibo dual-frequency pulsar polarimetry programs. Many of the RM
measurements were carried out toward the inner Galaxy and the Anticenter on
pulsars with no previous determination, while others are re-measurements
intended to confirm or improve the accuracy of existing values.
Stokes-parameter profiles are displayed for the 58 pulsars for which no
meaningful Stokes profile at lower frequency is available and four without a
high frequency pair. This is a population that includes many distant pulsars in
the inner Galaxy. A number of these polarized pulse profiles exhibit clear
interstellar-scattering tails; nonetheless, we have attempted to interpret the
associated emission-beam structures and to provide morphological
classifications and geometrical models where possible.
