We have reduced and tabulated photometry and polarimetry data at 2640 and 7500 ¿ observed by the Voyager 2 photopolarimeter experiment. Spatially resolved limb-to-terminator scans across Saturn's Equatorial Zone from 12¿ to 68¿ phase angle provide information on the altitude distribution of UV absorbing hazes and phase function and polarizing properties of stratospheric and tropospheric aerosols. Limb-to-terminator scans across the northern hemisphere at 10¿ phase angle are used to study altitude variations of the tropospheric cloud at several latitudes. For the Equatorial Zone we find (1) the UV photometryu and polarimetry are best fit by Rayleigh's pase matrix. (2) A stratospheric haze of small particles is allowed as long as the optical depth is near unity or less and the center of the haze differ significantly from models proposed by others. To be in agreement with ground based and other spacecraft data, the haze optical depth is about 0.4 at 2640 ¿ and decreases by a factor of 10 or more at 6400 ¿. If the haze aerosol scattering properties are similar to those for spheres with mean radius 0.1 &mgr;m, their imaginary refractive index 0.4 or larger at 2640 ¿ and the total column density above the tropopause is 109 cm-2, (3) UV contrasts between belts and zone are interpreted as altitude variations in the top of the tropospheric cloud. The altitudes derived here for three latitudes agree with alitude variations in the top of the tropospheric cloud. The altitudes derived here for three latitudes agree with altitudes derived from ground-based methane band studies and analyses of polarization from Pioneer 11. A high altitude absorber is abundant in the polar regions. (4) At 7500 ¿, the phase function of tropospheric aerosols in the Equatorial Zone is described by a synthetic two-term Henyey-Greenstein function with g1=0.54¿0.11, g2=-0.47¿0.08, f=0.87¿0.03, and Δ=0.986. The single scattering albedo in the North Equatorial Belt is Δ=0.967. The Equatorial Belt is Δ=0.967. The Equatorial Zone tropospheric aerosols are positively polarizing at all the phase angles of our observations.