A new model for the prediction of Dst on the basis of the solar wind

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Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms (2005, methodology): “…event t = 0 to the current moment t = t. Dynamical models similar to (1)–(3) were used earlier in a number of works to describe global loading-unloading processes in storms [Burton et al., 1975; Temerin and Li, 2002] and substorms [Baker et al., 1990; Klimas et al., 1992; Horton and Doxas, 1996].”
Dst model for 1995–2002 (2006, methodology): “[5] Our modeled Dst is a sum of the following six terms: Dst ¼ dst1*þ dst2*þ dst3*þ pressure termð Þ* þ direct IMF Bz termð Þ*þ offset termsð Þ: ð1Þ The terms dst1, dst2, dst3, (pressure term), and (direct Bz term) were all in our previous model [Temerin and Li, 2002].”
Energetic electrons, 50 keV to 6 MeV, at geosynchronous orbit: Their responses to solar wind variations (2005, methodology): “If we simply define geoeffectiveness in terms of the Dst index, VxBz is clearly the dominant controlling parameter [Burton et al., 1975; Temerin and Li, 2002].”