I collect emission-line profiles for seven intermediate polars, phase-resol
ved over the spin cycles. I then present the first systematic application o
f Doppler tomography to the spin cycles, with the aim of investigating whet
her spin-cycle tomography is a useful diagnostic tool. Four stars show line
emission from material falling onto both magnetic poles of the white dwarf
, but three others show line emission from only the upper pole. Tomography
can map the extent and shape of the line-emitting accretion curtains, but i
t can also give misleading results if the line flux changes significantly o
ver the spin cycle.