  We have performed integral field spectroscopy of the planetary nebulae Hen
3-1333 (PNG332.9-09.9) and Hen 2-113 (PNG321.0+03.9), which are unusual in
exhibiting dual-dust chemistry and multipolar lobes but also ionized by
late-type [WC 10] central stars. The spatially resolved velocity distributions
of the H$\alpha$ emission line were used to determine their primary
orientations. The integrated H$\alpha$ emission profiles indicate that Hen
3-1333 and Hen 2-113 expand with velocities of ~ 32 and 23 km/s, respectively.
The Hubble Space Telescope observations suggest that these planetary nebulae
have two pairs of tenuous lobes extending upwardly from their bright compact
cores. From three-dimensional geometric models, the primary lobes of Hen 3-1333
and Hen 2-113 were found to have inclination angles of about -30$^{\circ}$ and
40$^{\circ}$ relative to the line of sight, and position angles of
-15$^{\circ}$ and 65$^{\circ}$ measured east of north in the equatorial
coordinate system, respectively.
