  Frequency splitting coefficients from Global Oscillation Network Group (GONG)
and Michelson Doppler Imager (MDI) observations covering the period 1995--2001
are used to study temporal variations in the solar rotation rate at high
latitudes. The torsional oscillation pattern in the Sun is known to penetrate
to a depth of about $0.1R_\odot$ with alternate bands of faster and slower
rotating plasma. At lower latitudes the bands move towards equator with time.
At higher latitudes, however, the bands appear to move towards the poles. This
is similar to the observed pole-ward movement of large scale magnetic fields at
high latitudes. This also supports theoretical results of pole-ward moving
bands at high latitudes in some mean field dynamo models. The polar rotation
rate is found to decrease between 1995 and 1999 after which it has started
increasing.
