  Pulsar polarization profiles are very basic database for understanding the
emission processes in pulsar magnetosphere. After careful polarization
calibration of the 19-beam L-band receiver and verification of beam-offset
observation results, we obtain polarization profiles of 682 pulsars from
observations by the Five-hundred-meter Aperture Spherical radio Telescope
(FAST) during the survey tests for the Galactic Plan Pulsar Snapshot (GPPS)
survey and other normal FAST projects. Among them, polarization profiles of
about 460 pulsars are observed for the first time. The profiles exhibit diverse
features. Some pulsars have a polarization position angle curve with a good
S-shaped swing, and some with orthogonal modes; some have components with
highly linearly components or strong circularly polarized components; some have
a very wide profile, coming from an aligned rotator, and some have an
interpulse from a perpendicular rotator; some wide profiles are caused by
interstellar scattering. We derive geometry parameters for 190 pulsars from the
S-shaped position angle curves or with orthogonal modes. We find that the
linear and circular polarization or the widths of pulse profiles have various
frequency dependencies. Pulsars with large fraction of linear polarization are
more likely to have a large Edot.
