  We present the results of near continuous TESS optical observations of the
asynchronous polar CD Ind (RX J2115-5840). The 27.9 d long light curve, with 2
min resolution, reveals remarkable changes in the magnetic accretion geometry
of the system over the 7.3 d beat period. We have modelled the changes in the
optical spin period pulse shape using a cyclotron emission mapping technique.
The resulting cyclotron emission maps of the magnetic white dwarf reveal how
the accretion geometry changes from single to two pole accretion and back over
the beat cycle. Finally, we present the results from particle based numerical
magnetic accretion simulations, that agree with our interpretation of the
changing accretion scenario.
