Statistical analysis of bursty bulk flows, plasma bubbles, and their wakes using Cluster and Double Star

Details Statistical analysis of bursty bulk flows, plasma bubbles, and their wakes using Cluster and Double Star Statistical analysis of bursty bulk flows, plasma bubbles, and their wakes using Cluster and Double Star

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm41a1847f&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM41A-1847

Physics

[2744] Magnetospheric Physics / Magnetotail, [2760] Magnetospheric Physics / Plasma Convection, [2790] Magnetospheric Physics / Substorms

Scientific paper

It has previously been shown that bursty bulk flows (BBFs) and plasma bubbles transport significant levels of magnetic flux through the magnetotail. They are thought to be closely linked with substorm onset and dipolarization of the inner magnetosphere; directly linked with auroral streamers through field-aligned currents; and displace the surrounding plasma creating wakes behind them. Using data from the Cluster and Double Star spacecraft, we statistically examine the properties and effects of BBFs and plasma bubbles in the magnetosphere.

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