A study of riometer, photometer, and ionosonde data from South Pole Station has revealed a class of unusual dayside absorption events which occur near local magnetic noon when South Pole is located poleward of the dayside cusp. These events, which can reach values in excess of 1 dB in narrow-beam 38.2-MHz riometer measurements, are accompanied by significant enhancement of the O(1D2) 630.0-nm emission. However, because there is no corresponding change in the N2+ 427.8-nm emission, it is unlikely that these events are caused by the conventional D or lower E region ionization increases usually attributed to the precipitation of auroral electrons of keV energy. Rather, the comparison of South Pole imaging riometer and ionosonde data with simultaneous Halley PACE HF radar data suggests that these unusual absorption events are related to F region electron density structures drifting from the dayside oval into the polar cap. If further work sustains this interpretation, then new prospects will be opened up for using imaging riometers to examine aspects of polar cap convection. ¿ American Geophysical Union 1993