Physics
Scientist
ISAS, University of Saskatchewan, 116 Science Place, Saskatoon, SK S7N 5E2, Canada
A possible origin of dayside Pc1 magnetic pulsations observed at high latitudes
IMF By effects in the magnetospheric convection on closed magnetic field lines
Ionospheric convection in the postnoon auroral oval: Super Dual Auroral Radar Network (SuperDARN) and polar ultraviolet imager (UVI) observations
Meridional motions of the afternoon radar aurora, auroral electrojets, and absorption patches under variable IMF conditions
On the motion of dayside auroras caused by a solar wind pressure pulse
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