The response of the near-earth magnetotail to a sharp and isolated nor
thward turning of the IMF observed at the WIND spacecraft is studied i
n the near-Earth plasma sheet at x=-19 Re. Because of the possible tim
e coincidence this northward turning could be causally related to an o
nset of the substorm expansion phase where Bz increased and the earthw
ard convection intensified in the plasma sheet. The changes in the flo
w velocity and Bz to lower values occurred about 30 min later but they
were not associated with an expansion phase onset. Thus the observati
ons do not support the suggestion that the northward IMF turning produ
ces a tailward sweep of the reduced dawn-to-dusk electric field and th
ereby triggers the substorm onset.