Continuous observation of cusp auroral dynamics in response to an IMF BY polarity change

Physics – Plasma Physics

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Magnetospheric Physics: Auroral Phenomena, Magnetospheric Physics: Solar Wind/Magnetosphere Interactions, Space Plasma Physics: Magnetic Reconnection

Scientific paper

The IMF BY control of the motion pattern and the location of cusp auroral activity has been continuously monitored in a case when the BY component of the interplanetary magnetic field (IMF) went from -15 nT to +15 nT in the course of 20 minutes. This is the first time a direct observation of an IMF BY regulated shift in the longitudinal position of the auroral cusp has been documented. The IMF BY regulation of the cusp is regarded to be a unique signature of magnetopause reconnection. In this particular case the zonal shift of the cusp center is estimated to be at least 3 hours in magnetic local time. The observations indicate that the cusp reconfigured within a few minutes after the BY polarity change imposed on the magnetopause.

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