Using intermediate degree p-mode frequency data sets for solar cycle 22, we
find that the frequency shifts and magnetic indices show a 'hysteresis' ph
enomenon. It is observed that the magnetic indices follow different paths f
or the ascending and descending phases of the solar cycle, as the descendin
g path always seems to follow a higher track than the ascending one. Howeve
r, for the radiative indices, the paths cross each other indicating phase r
eversal.