Measurements of the relative phases of pulses in separate energy bands
provide important information about the geometry of pulsars' emission
regions. The lack of pulsars detected in different wave bands has ham
pered this approach in the past. Here we present an analysis of ROSAT
data on Geminga and give the phase relationship between the X-ray and
MeV-GeV lightcurves. The X-ray emission is sinusoidal and maximizes ju
st before the second gamma-ray peak.