  We present preliminary results from our investigation into using an
'inside-out' velocity space for creating a Doppler tomogram. The aim is to
transpose the inverted appearance of the Cartesian velocity space used in
normal Doppler tomography. In a comparison between normal and inside-out
Doppler tomograms of cataclysmic variables, we show that the inside-out
velocity space has the potential to produce new insights into the accretion
dynamics in these systems.
