Improvements to the HAF solar wind model for space weather predictions

By C. Fry, Wei Sun, C. Deehr, M. Dryer, Z. Smith, S. Akasofu, M. Tokumaru, M. Kojima. 2001

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Radiation Belt Environment model: Application to space weather nowcasting (2008, methodology): “Solar wind models of this kind have been established or are under development [Fry et al., 2001; Detman et al., 2006].”
Kp forecast models (2005, methodology): “, the HakamadaAkasofu-Fry (HAF) code [Fry et al., 2001; Hakamada and Akasofu, 1982] and the Wang-Sheeley model [Wang”
Deriving the radial distances of wide coronal mass ejections from elongation measurements in the heliosphere - application to CME-CME interaction (2009, methodology): “2 model of Hakamada and Akasofu (1982) and Fry et al. (2001) have also been performed and published in Webb et al. (2009). Based on the numerical analyses, the fronts observed by HI2 and SMEI have been associated with the two CMEs, validating the numerical models on one hand and helping the analysis”