  IP Pegasi is an eclipsing dwarf nova lying above the period gap with an
orbital period of 3.8h. It is the first cataclysmic variable to show evidence
of spiral arms in its accretion disc. We present new time-resolved echelle
spectroscopic observations of IP Peg, covering the 3900-7700 Angstrom range.
This allows us to produce simultaneous Doppler Maps in 9 emission lines.
