The Crab Pulsar (PSR B0531+21) was observed by the four Narrow Field I
nstruments onboard the Italian-Dutch satellite BeppoSAX in August and
September 1996, during the Science Verification Phase. The fine time r
esolution (15 mu s) and high statistics provided phase histograms of v
ery good quality over the entire energy band (0.1-300 keV) covered by
BeppoSAX payload. In this letter we present a detailed study of the va
riations in the light curve shape with energy and evaluate the spectra
l index difference between the main features.