Coronal Shocks and Solar Energetic Proton Events

By E. Cliver, S. Kahler, D. Reames. 2004

223 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/bdf30333cf99fed2bcfa5384c70d5ad00ebba560

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Nat Gopalswamy
2. M. Temmer
3. S. Yashiro
4. D. Reames
5. R. Howard
6. N. Lugaz
7. S. Akiyama
8. A. Vourlidas

In Geophysics

1. M. Temmer
2. Nat Gopalswamy
3. Martin A. Lee
4. D. Reames

Citations in the corpus

• The Two Sources of Solar Energetic Particles (2012, background): “Separately, Cliver, Kahler, and Reames (2004) found that (non-GLE) SEP events were most strongly correlated with 1-14 MHz type II radio emission corresponding to acceleration above ~3 solar radii.”
• Type II radio bursts and energetic solar eruptions (2003, background): “This longitude dependence was also shown recently by Cliver et al. [2004] for m-to-DH events.”
• 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).”
• SOLAR RELEASE TIMES OF ENERGETIC PARTICLES IN GROUND-LEVEL EVENTS (2009, background): “Cliver et al. (2004) found that SEP events were much more strongly correlated with type II radio bursts (a proxy for shock waves) beginning at decametric frequencies corresponding ∼ 3 RS than with metric type II bursts with starting frequencies corresponding to ∼ 1.5 RS.”
• Coronal mass ejections and other extreme characteristics of the 2003 October–November solar eruptions (2005, result): “This is a relatively high ratio (69%) compared with 36–38% for the 1996–2002 period [Gopalswamy et al., 2004a; Cliver et al., 2004a ].”
• Coronal mass ejections of solar cycle 23 (2006, background): “The SEP events are also closely related to type II radio bursts (Gopalswamy 2003; Cliver et al. 2004) since the same shocks accelerate SEPs and electrons.”
• Coronal mass ejections, type II radio bursts, and solar energetic particle events in the SOHO era (2008, background): “Statistical studies have confirmed this close association (see e.g. Gopalswamy, 2003; Cliver et al., 2004a).”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…divided into impulsive events of shorter duration, most often associated with solar flares but not always (Kahler, Reames, and Sheeley, 2001) and gradual events, most often associated with CME-driven shocks (Cane, McGuire, and von Rosenvinge, 1986; Reames, 1999; Cliver, Kahler, and Reames, 2004).”