Slow-Rise and Fast-Rise Phases of an Erupting Solar Filament, and Flare Emission Onset

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Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts (2008, background): “Only a few studies compared directly the kinematics of prominence/filament eruptions and associated HXR bursts (Kahler et al. 1988; Sterling & Moore 2004, 2005).”
Eruption of magnetic flux ropes during flux emergence (2008, unknown): “Typically, CMEs exhibit three distinct phases (Zhang et al. 2001): an initiation phase, often observed as the slow rise of a filament (e.g. Sterling & Moore 2005; Schrijver et al. 2008), a rapid acceleration phase, and a propagation phase at approximately constant velocity.”
A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections (2006, background): “Individual events with normal accelerations have been reported by many studies (Wood et al. 1999; Shanmugaraju et al. 2003; Qiu et al. 2004; Vršnak et al. 2004; Kundu et al. 2004; Sterling & Moore 2005).”
An Observational Overview of Solar Flares (2011, background): “…explicitly linked pre-flare brightenings with the destabilization of the magnetic structure that will lead to a CME (e.g., Harrison et al. 1985; Sterling & Moore 2005) or a filament eruption (Fárnı́ket al. 2003; Chifor et al. 2007; Liu et al. 2009d) although coronagraphic studies of the…”