Coronal Mass Ejections Associated with Impulsive Solar Energetic Particle Events
By S. Kahler, D. Reames, N. R. Sheeley. 2001
175 citations recorded by the source corpus.
Subfields: Artificial Intelligence, Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/4be670ed5d1a5acd4dd66379244c763b4ffb88c2
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Citations in the corpus
- Magnetic Topology of Impulsive and Gradual Solar Energetic Particle Events (2002, methodology): “This diagram is similar to the ones considered by Kahler et al. (2001) for impulsive SEP events with CMEs and was proposed by Shimojo & Shibata (2000) to describe X-ray jets and the source of the 10–100 keV electrons that produce interplanetary type III radio bursts (Robinson & Benz 1998).”
- The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “Historically, SEPs have been 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,…”
- A Model for Spectral and Compositional Variability at High Energies in Large, Gradual Solar Particle Events (2006, background): “…both impulsive and gradual events (Mason et al. 1999, 2002), made possible by the better isotopic resolution and increased collecting power in the new particle instruments; and (2) the discovery of generally smaller and slower CMEs that sometimes accompany impulsive SEP events (Kahler et al. 2001).”
- The Two Sources of Solar Energetic Particles (2012, background): “A few larger impulsive SEP events have been associated with narrow CMEs that may represent material ejected upward from the reconnection site of a jet (Kahler, Reames, and Sheeley 2001).”
- Coronal Holes, Jets, and the Origin of 3He-rich Particle Events (2006, background): “However, Kahler et al. (2001) showed that the injection time of an impulsive SEP event on 2000 May 1 (as deduced from the difference in arrival times between the 2 and 20 MeV protons) coincided approximately with the emer- gence of a fast ( 1000 km s 1), narrow (P20 ) white-light CME above the…”