We present a new method to map the surface brightness of the accretionstreams in AM Herculis systems from observed light curves. Extensive tests ofthe algorithm show that it reliably reproduces the intensity distribution ofthe stream for data with a signal-to-noise ratio >5. As a first application, wemap the accretion stream emission of Civ lambda 1550 in the polar UZ Fornacisusing HST FOS high state spectra. We find three main emission regions along theaccretion stream: (1) On the ballistic part of the accretion stream, (2) on themagnetically funneled stream near the primary accretion spot, and (3) on themagnetically funneled stream at a position above the stagnation region
