  We use helioseismic data obtained over two solar cycles to determine whether
there are changes in the near-surface shear layer (NSSL). We examine this by
determining the radial gradient of the solar rotation rate. The radial gradient
itself shows a solar-cycle dependence, and the changes are more pronounced in
the active latitudes than at adjoining higher latitudes; results at the highest
latitudes (greater than about70 degrees) are unreliable. The pattern changes
with depth, even within the NSSL. We find that the near-surface shear layer is
deeper at lower latitudes than at high latitudes and that the extent of the
layer also shows a small solar-cycle related change.
