Coronal Holes, Jets, and the Origin of 3He-rich Particle Events

By Y. Wang, M. Pick, G. Mason. 2006

169 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/1a370143c6a5aa151122441fb19c495c2422299f

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In Astronomy and Astrophysics

Citations in the corpus

A Model for Spectral and Compositional Variability at High Energies in Large, Gradual Solar Particle Events (2006, background): “Impulsive events, on the other hand, are generally ascribed to particle acceleration at sites associated with flares, probably through resonant wave-particle interactions followingmagnetic reconnection (Reames 2002; Wang et al. 2006).”
THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “…noted in numerous studies of surges (e.g., Asai et al. 2001; Chen et al. 2008), chromospheric Ca ii H jets (Morita et al. 2010), EUV jets (Chae et al. 1999; Wang et al. 2006; Jiang et al. 2007; Gontikakis et al. 2009), and X-ray jets (Kim et al. 2001; Chifor et al. 2008a, 2008b; Kamio et al. 2010).”
The Two Sources of Solar Energetic Particles (2012, background): “Conversely, impulsive SEP events seen at 1 AU are commonly associated with jets (Wang, Pick, and Mason 2006; Nitta et al. 2006), where reconnection between open and closed field lines takes place (e.g. Shibata, et al. 1992; Heyvaerts, Priest, Rust 1977; Shimojo and Shibata 2000; Aschwanden (2002);…”
Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation (2016, methodology): “Among the mechanisms that could allow the flare-accelerated particles to escape are interchange reconnection (Wang et al. 2006) between open and closed field lines, which can occur at neutral points (Fisk 1996), and even more frequently at component reconnection sites at coronal hole boundaries (Rap”