Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model

By B. Vršnak, T. Žic, D. Vrbanec, M. Temmer, T. Rollett, Christian Möstl, Astrid Veronig, J. Čalogović, M. Dumbović, S. Lulić and 2 more. 2013

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ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, background): “…by a viscous drag force (as solar gravity can be neglected), which is proportional to a drag coefficient, the CME cross section, the ambient solar wind density, and the square of the velocity difference between the CME and the solar wind (e.g., Cargill 2004; Vršnak et al. 2013; Žic et al. 2015).”
CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU (2014, background): “Especially for very fast CMEs, these speeds will not match the speeds measured in situ at 1 AU because of the CME deceleration that occurs up to 1 AU (e.g. Gopalswamy et al. 2001; Vršnak et al. 2013).”
The Physical Processes of CME/ICME Evolution (2017, methodology): “After being proposed in its initial form by Vršnak and Gopalswamy (2002), the formulation of the basic form of DBM, suited for space-weather forecasting, was completed by Vršnak et al. (2013).”