Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsm13c..07e&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SM13C-07
Physics
2431 Ionosphere/Magnetosphere Interactions (2736), 2463 Plasma Convection (2760), 2706 Cusp, 2723 Magnetic Reconnection (7526, 7835), 2724 Magnetopause And Boundary Layers
Scientific paper
High-latitude reconnection tailward of the cusps is predicted to occur during northward IMF. Northward IMF conditions are also regarded favorable in generating convection patterns that deviate from the classical 2-cell system in the polar cap ionosphere. We here present evidence in favor of this scenario on the basis of Cluster and SuperDARN joint observations on 14 February 2003 when Cluster traversed the high-latitude region of the northern cusp into the magnetosheath. The IMF measured by Cluster in the magnetosheath is Bx<0, By>0, Bz>0 and By>Bz. As predicted during positive IMF By and Bz, the SuperDARN radars observe enhanced sunward and dawnward convective flow across the noon meridian at the Cluster footprint. The enhanced ion velocity observed simultaneously at Cluster is also directed sunward and dawnward with a dominant convective component in the dawnward direction. The ion velocity at Cluster satisfies the shear-stress balance test and suggests a lobe reconnection site tailward and duskward of Cluster in agreement with the results of an MHD simulation performed during this event.
Balogh André
Dunlop Malcolm W.
Ergun Robert E.
Eriksson Samantha
Gosling Jack T.
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