Solar flares, type III radio bursts, coronal mass ejections, and energetic particles

By H. Cane, W. Erickson, N. Prestage. 2002

145 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/3b96006123d5757174b4cbc77d6db7fdb6f06afb

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. D. Reames
2. Nat Gopalswamy
3. S. Yashiro
4. Martin A. Lee
5. H. Cane
6. I. G. Richardson
7. S. Akiyama
8. P. Mäkelä

In Geophysics

1. D. Reames
2. Nat Gopalswamy
3. Martin A. Lee
4. E. Cliver
5. S. Kahler
6. Philip J. Erickson
7. Anthea J. Coster
8. I. Usoskin

Citations in the corpus

• Coronal Shocks and Solar Energetic Proton Events (2004, methodology): “…from Švestka et al. (1980) shows that particles accelerated in this manner, particularly those accelerated late relative to the start of the flare as required by the Cane et al. (2002) definition of type III-l emission, can serve as seed particles for a shock upon escaping the confines of the CME.”
• Coupled Hydromagnetic Wave Excitation and Ion Acceleration at an Evolving Coronal/Interplanetary Shock (2005, background): “However, type III radio bursts show that electrons do escape to open field lines (see x 8.5; Cane et al. 2002).”
• A review of solar type III radio bursts (2014, background): “It has been suggested (Cane et al., 2002) that type III-l bursts are produced by electrons accelerated by reconnection behind fast CMEs.”
• A study of solar energetic particle events of 1997–2006: Their composition and associations (2010, background): “They confirm the result from an earlier study [Cane et al., 2002] that essentially all events have associated type III emissions and that for the largest events these start or extend beyond the maximum of the flare emissions, i.”
• Properties of Ground Level Enhancement Events and the Associated Solar Eruptions During Solar Cycle 23 (2012, methodology): “Cane et al. (2002) suggested that the complex type III bursts are indicative of large SEP events.”
• Science with the Murchison Widefield Array (2012, background): “The active Sun produces both broadband (∆f/f ≈ 1) and narrowband (∆f/f 10−2) emissions at frequencies from below 1 MHz to approximately 30 GHz (e.g., Wild et al. 1963; Bastian et al. 1998; Cane et al. 2002; Karlický 2003; Cairns 2011).”
• Shock Geometry, Seed Populations, and the Origin of Variable Elemental Composition at High Energies in Large Gradual Solar Particle Events (2005, background): “According to Cane et al. (2002), the source region for this event was at E95 , behind the east limb.19 At 1 MeV nucleon 1, Fe/C is suppressed relative to the corona.”