A statistical look at plasmaspheric drainage plumes

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EMIC wave activity during geomagnetic storm and nonstorm periods: CRRES results (2010, background): “This does not show conclusively that (on average) EMIC waves during storms occurred in the plasmasphere or in plasmaspheric plumes, but it is consistent with the number densities we would expect to see if a plume were present [ Borovsky and Denton, 2008 ].”
Low‐energy ions: A previously hidden solar system particle population (2012, background): “Densities are typically 10–100 cm 3 and fluxes 10(25) to 10(27) ions/s, much of which is lost via dayside reconnection [Chandler et al., 1999; Moore et al., 2008; Darrouzet et al., 2008, 2009; Borovsky and Denton, 2008; Spasojevic and Sandel, 2010].”
Plasmaspheric Density Structures and Dynamics: Properties Observed by the CLUSTER and IMAGE Missions (2009, background): “These global observations of plasmaspheric phases provide context for many in situ plume studies that have been performed (Garcia et al. 2003; Chen and Moore 2006; Darrouzet et al. 2006a; Borovsky and Denton 2008; Darrouzet et al. 2008).”