Traveling Compression Regions and Current Disruptions: A Cluster Perspective

Details Traveling Compression Regions and Current Disruptions: A Cluster Perspective Traveling Compression Regions and Current Disruptions: A Cluster Perspective

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsm11d..03m&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SM11D-03

Physics

2463 Plasma Convection (2760), 2723 Magnetic Reconnection (7526, 7835), 2744 Magnetotail, 7954 Magnetic Storms (2788)

Scientific paper

TCR and current disruptions have quite frequently been confused. Cluster data allow to make a clear difference between these two phenomena in terms of duration and propagation characteristics. We present detailed case studies of plasma and magnetic field changes associated with both signatures and of the simultaneous plasma convection in the lobes of the magnetotail. These multi spacecraft measurements are used to compute quantitative features of the dynamics of the tail after substorm onsets.

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