A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES

By J. Drake, P. Cassak, M. Shay, M. Swisdak, E. Quataert. 2009

158 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a7a7f8133a43c71871190cb185b50027c0f19fc4

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In Astronomy and Astrophysics

Citations in the corpus

THE VECTOR DIRECTION OF THE INTERSTELLAR MAGNETIC FIELD OUTSIDE THE HELIOSPHERE (2010, background): “Observations (Lin et al. 2003) and simulations (Drake et al. 2009) have demonstrated that reconnection can energize ions (this occurs in addition to the electric energization necessary for the 2-3 kHz radio emission).”
Solar Orbiter (2012, background): “In this case, particles can be accelerated for hours, and may ‘leak’ around the CME structure and become mixed with the shock-accelerated particles (Lin, 2006; Cargill et al., 2006; Drake et al., 2009).”
The Two Sources of Solar Energetic Particles (2012, background): “These and most subsequent models relate impulsive SEP events directly to the fundamental physics of magnetic reconnection and, hence, to flares ( .g. Drake et al. 2009).”
The FIP and Inverse FIP Effects in Solar and Stellar Coronae (2015, background): “Equating this to the pitch diffusion coefficient, D = (π/4)Ωs ( δB2/B2 ) , 1 This is similar to the case in Drake et al. (2009), where pick-up ion behavior leads to mass dependent fractionation. where δB is the magnetic field perturbation due to the wave, and B is the ambient magnetic field, we…”
Non-thermal particle acceleration in collisionless relativistic electron-proton reconnection (2016, background): “Nonthermal particle acceleration in plasma processes has been studied within fluid (e.g., magnetohydrodynamic, MHD) frameworks by tracking distributions of passive test particles (Nodes et al. 2003; Onofri et al. 2006; Drake et al. 2009; Ding et al. 2010; Gordovskyy et al. 2010; Kowal et al. 2011).”