An empirical phase space analysis of ring current dynamics: Solar wind control of injection and decay

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Solar and interplanetary sources of major geomagnetic storms during 1996–2002 (2004, neutral): “[1975] [e.g., Feldstein, 1992; Fenrich and Luhmann, 1998; O’Brien and McPherron, 2000].”
Dst of the Carrington storm of 1859 (2006, methodology): “(5)) with the O Brien and McPherron (2000) specification of”
A 21st Century View of the March 1989 Magnetic Storm (2019, methodology): “Using empirical relations from Cliver et al. (1990), O'Brien and McPherron (2000), and Nagatsuma et al. (2015), the shock speed and the Dst variation are used to estimate the solar wind speed and Bs during 13 and 14 March.”
Major geomagnetic storms (Dst<=-100~nT) generated by corotating interaction regions in 1996--2004 (2006, background): “The O’Brien and McPherron [2000] equations, which estimate Dst by integrating the incident solar wind electric field and incorporat-”
Properties and geoeffectiveness of magnetic clouds in the rising, maximum and early declining phases of solar cycle 23 (2005, methodology): “Figure 12 shows the predictedD st development according to the O’Brien and McPherron (2000a) and Wang et al.”