Abstract. Floating ice shelves buttress the Antarctic Ice Sheet,
which is losing mass rapidly mainly due to ocean-driven melting and the
associated disruption to glacial dynamics. The local ocean circulation near
ice shelves is therefore important for the prediction of future ice mass
loss and related sea-level rise as it determines the water mass exchange,
heat transport under the ice shelf and resultant melting. However, the
dynamics controlling the near-coastal circulation are not fully understood.
A cyclonic (i.e. clockwise) gyre circulation (27 km radius) in front of the
Pine Island Ice Shelf has previously been identified in both numerical
models and velocity observations. Mooring data further revealed a potential
reversal of this gyre during an abnormally cold period. Here we present
ship-based observations from 2019 to the west of Thwaites Ice Shelf,
revealing another gyre (13 km radius) for the first time in this habitually
ice-covered region, rotating in the opposite (anticyclonic, anticlockwise)
direction to the gyre near Pine Island Ice Shelf, despite similar wind
forcing. We use an idealised configuration of MITgcm, with idealised forcing
based on ERA5 climatological wind fields and a range of idealised sea ice
conditions typical for the region, to reproduce key features of the observed
gyres near Pine Island Ice Shelf and Thwaites Ice Shelf. The model driven
solely by wind forcing in the presence of ice can reproduce the horizontal
structure and direction of both gyres. We show that the modelled gyre
direction depends upon the spatial difference in the ocean surface stress,
which can be affected by the applied wind stress curl filed, the percentage
of wind stress transferred through the ice, and the angle between the wind
direction and the sea ice edge. The presence of ice, either it is fast
ice/ice shelves blocking the effect of wind or mobile sea ice enhancing the
effect of wind, has the potential to reverse the gyre direction relative to
ice-free conditions.