Propagation Characteristics of Plasma Sheet Oscillations During a Small Storm

Details Propagation Characteristics of Plasma Sheet Oscillations During a Small Storm Propagation Characteristics of Plasma Sheet Oscillations During a Small Storm

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm23a1176g&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM23A-1176

Physics

2700 Magnetospheric Physics (6939), 2764 Plasma Sheet, 2772 Plasma Waves And Instabilities (2471), 2788 Magnetic Storms And Substorms (7954), 2794 Instruments And Techniques

Scientific paper

On March 24, the THEMIS spacecraft were in a string-of-pearls configuration through the dusk plasma sheet at the recovery phase of a small storm. Large undulations of the plasma sheet were observed that brought the 5 probes from one lobe to another. Each neutral sheet crossing was accompanied by fast flows and Pi2 oscillations, which are the topic of a companion paper. In this paper we focus on the low frequency (~10min) large scale plasma sheet undulations and determine their propagation characteristics, origin, properties and their importance for the dynamic evolution of the tail in the presence of storm-time substorms.

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