Physics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsm23c..02e&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SM23C-02
Physics
2463 Plasma Convection (2760), 2706 Cusp, 2776 Polar Cap Phenomena, 2784 Solar Wind/Magnetosphere Interactions
Scientific paper
We use the Cluster string of pearl configuration in the mid-altitude polar cusp to investigate temporal variations of the polar cusp. On 7 Aug. 2004, Cluster 4 was moving poleward through the Northern cusp, followed by Cluster 1 about 3 min later, Cluster 2 about 9 min later and finally Cluster 3 about 18 min later. The ACE spacecraft detected a Southward IMF turning before the cusp crossings and Bz stayed negative throughout. Cluster 4 observed a staircase ion dispersion with 2 steps, a high energy one around 1 keV at low latitude and a low energy one at higher latitude. C1 around 3 min later did not observe the high energy step anymore but a dispersion with a low energy cut-off more or less continuous through the cusp. About 18 min later, C3 observed a new dispersion on the equatorward side of the cusp detached from the main cusp precipitation. The observations will be compared with the predictions from a three-dimensional magnetohydrodynamic (MHD) simulation. This event will then be discussed in term of temporal evolution of newly reconnected field lines on the equatorward side of the cusp under IMF-Bz negative.
Berchem Jean
Bosqued Jean Michel
Dandouras Iannis
Dunlop Malcolm
Escoubet Christophe P.
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