Energetic particle acceleration and transport at coronal mass ejection–driven shocks

By Gang Li, Gary Zank, W. Rice. 2003

171 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c78a65ff02b3a0df5a0432407db2626c67d5a062

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In Astronomy and Astrophysics

1. D. Reames
2. Martin A. Lee
3. Nat Gopalswamy
4. M. Temmer
5. A. Tylka
6. A. Vourlidas
7. Brian R. Dennis
8. A. Emslie

Citations in the corpus

• Coronal Mass Ejection Shock and Sheath Structures Relevant to Particle Acceleration (2005, unknown): “Recent time-dependent calculations of shockdriven solar energetic particle (SEP) acceleration have relied on spherically symmetric shock propagation models that do not include CME initiation or interaction of the shock with a structured solar wind (Zank et al. 2000; Li et al. 2003; Lario 1998).”
• STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, unknown): “Several efforts described in the literature (e.g. Lario et al. 1998; Li et al. 2003) make use of MHD model simulations of interplanetary shocks as the basis for SEP spatial distribution and time profile descriptions that can be compared to multipoint or single spacecraft observations.”
• A brief review of “solar flare effects” on the ionosphere (2009, methodology): “Details of the models are described by Zank et al. [2000, 2007], Li et al. [2003, 2005] , and Verkhoglyadova et al. [2009].”
• Shock Geometry, Seed Populations, and the Origin of Variable Elemental Composition at High Energies in Large Gradual Solar Particle Events (2005, background): “…are shocks driven by fast coronal mass ejections (CMEs), are productive opportunities for refining our understanding of shock acceleration (Reames 1999; Lee 2000, 2005; Zank et al. 2000; Rice et al. 2003; Cliver et al. 2004) and particle transport (Ng et al. 1999, 2003; Li et al. 2003).”
• Particle acceleration at perpendicular shock waves: Model and observations (2005, methodology): “[20] By taking the following three steps, we can utilize our earlier approaches [Zank et al., 2000; Li et al., 2003] directly.”
• Energy partition in two solar flare/CME events (2004, methodology): “Simulations by J. Giacalone (personal communication, 2002) [see also Li et al., 2003] using scattering mean free paths of 0.01 to 1 AU indicate that the probability of crossing 1 AU more than once is energy dependent, with A10104 EMSLIE ET AL.”
• Coupled Hydromagnetic Wave Excitation and Ion Acceleration at an Evolving Coronal/Interplanetary Shock (2005, methodology): “…theoretical treatments of SEP acceleration and transport in gradual events: the seminumerical theory of Zank and coworkers (Zank et al. 2000; Rice & Zank 2003; Rice et al. 2003; Li et al. 2003) is described in x 1, while the numerical theory of Ng et al. (1999, 2001, 2003) is described in x 6.”