A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections

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Numerical simulations of fast and slow coronal mass ejections (2007, background): “However, the data always showed a continuous distribution of velocities with a single peak (Zhang & Dere 2006 and references therein).”
Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts (2008, background): “However, this phase is the most interesting one for the CME dynamics, since in the outer corona the CMEs might be already adjusted to the solar wind speed or show just some “residual acceleration” (Chen & Krall 2003; Zhang & Dere 2006).”
Properties of Ground Level Enhancement Events and the Associated Solar Eruptions During Solar Cycle 23 (2012, methodology): “The acceleration given by (5) is similar to the one used by Zhang and Dere (2006).”
Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, background): “Recently, Zhang & Dere (2006) cataloged a broad distribution of magnitudes of the rapid acceleration phase, from 2.8 to 4400 m s 2, and derived a scaling law for the peak acceleration as a function of the duration of acceleration phase.”
COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “Several authors found a correlation between the CME acceleration and the flare soft X-ray emission (Zhang et al. 2001, 2004; Zhang & Dere 2006; Vršnak et al. 2004; Maričić et al. 2007; Vršnak et al. 2007).”