Lobe Cell Convection and Polar cap Precipitation

Physics

Scientific paper

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2475 Polar Cap Ionosphere, 2704 Auroral Phenomena (2407), 2784 Solar Wind/Magnetosphere Interactions, 2455 Particle Precipitation, 2463 Plasma Convection

Scientific paper

The characteristic electric and magnetic field signature of lobe cells as observed by the low-altitude FAST satellite are compared with Polar ultraviolet images of polar cap auroral activity. Initial results suggest that there is an intimate coupling between the sunward flow of the lobe cell and transpolar auroral arcs or diffuse polar cap precipitation. However, in some cases where the fields signature is suggestive of lobe cell convection, there is no detectable particle precipitation in the sunward flowing part of the lobe cell. Moreover, the presence of eveningside lobe cells occasionally coincide with UV data intensifications in the pre-midnight 2100 MLT quadrant and/or the post-noon 1500 MLT quadrant. The magnetic local time dependence of the lobe cells and polar cap precipitation on the interplanetary magnetic field are examined using the upstream ACE and Wind monitors. The relative importance of the By and Bz components are investigated and compared with the predictions of the antiparallel merging model.

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