  We present the results of applying our inside-out velocity projection and
flux modulation mapping techniques to the Doppler tomography of magnetic
cataclysmic variables. The inside-out tomogram is constructed by directly
projecting phase-resolved spectra onto the inside-out framework. In addition,
our flux modulation mapping technique extracts any information related to the
modulation of the line flux by utilising consecutive half-phase tomograms. We
apply this to both the standard and the inside-out techniques. Our test cases,
the polars HU Aqr and V834 Cen, and the intermediate polar PQ Gem, were chosen
because of their known accretion characteristics, namely ballistic, magnetic
and curtain dominated accretion, respectively. In all three cases the
inside-out tomogram better exposes low-velocity emission details which are
overly compacted in the standard tomogram. This is especially apparent for the
mid-inclination V834 Cen where the almost blob-like blended lower velocity
emission in the standard tomogram is more exposed in the inside-out tomogram,
making it easier to distinguish between the ballistic and magnetically confined
accretion flows that are evident in the trailed spectra. Similarly, the
inside-out tomogram enhances high velocity emission details which are washed
out in the standard tomogram. This is particularly effective in revealing the
high velocity magnetic accretion flows in the polars HU Aqr and V834 Cen. The
addition of our flux modulation technique gives a significant improvement in
reproducing the trailed input spectra adding more confidence to the
interpretation of the Doppler maps. Furthermore, amplitude and phase maps are
constructed that further reveal amplitude and phasing characteristics of the
emission components in the three test cases.
