The role of the foreshock or quasi parallel shock in causing motions o
f the magnetopause is studied using both the number of crossings of th
e magnetopause found as ISEE 1 and 2 passed through the expected regio
n of the magnetopause on each orbit and by determining the minimum and
maximum distances to the magnetopause on each pass. Downstream of the
afternoon magnetosheath and bow shock, a region free from foreshock e
ffects for typical interplanetary magnetic field (IMF) directions, the
north-south component of the IMF controls these motions. On the morni
ng side additional oscillation in the magnetopause position is found f
or both northward and southward IMF. We interpret these increased moti
ons as driven by the pressure variations in and behind the foreshock r
egion or quasi-parallel shock. These results are consistent with other
studies of foreshock effects on the magnetosphere which show little e
ffect On erosion of the magnetopause or flux transfer event occurrence
.