Bulk plasma properties at geosynchronous orbit.

By M. Denton, M. Thomsen, H. Korth, S. Lynch, Jiajun Zhang, M. Liemohn. 2005

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Geomagnetic storms driven by ICME- and CIR-dominated solar wind (2006, methodology): “Large changes in composition between solar maximum and solar minimum are known to occur in the ionosphere [e.g., Heelis et al., 1990; West et al., 1997; Denton and Bailey, 2001], and such compositional changes may be reflected in the inner magnetosphere and plasma sheet composition [e.g., Young et a”
Circulation of Heavy Ions and Their Dynamical Effects in the Magnetosphere: Recent Observations and Models (2014, methodology): “7 index) on the O+ ion density in the plasma sheet was provided by Young et al. (1982), Lennartsson and Shelley (1986), Lennartsson (1989), Denton et al. (2005), Nosé et al. (2009), Mouikis et al. (2010), Ohtani et al. (2011) and Maggiolo and Kistler (2014).”
THEMIS analysis of observed equatorial electron distributions responsible for the chorus excitation (2010, methodology): “Denton et al. [2005] performed a statistical analysis using LANL data in the geosynchronous orbit and found that the anisotropy of hot electrons (30 eV–45 keV) on the dayside was generally larger than that on the nightside.”