THE LONGITUDINAL PROPERTIES OF A SOLAR ENERGETIC PARTICLE EVENT INVESTIGATED USING MODERN SOLAR IMAGING

By A. Rouillard, N. Sheeley, A. Tylka, A. Vourlidas, C. Ng, C. Rakowski, C. Cohen, R. Mewaldt, G. Mason, D. Reames and 3 more. 2011

158 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/fe320c2142ff3b8801b7dd828ee0f0ea60aa0fa7

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In Astronomy and Astrophysics

1. M. Temmer
2. H. Cane
3. I. G. Richardson
4. N. Lugaz
5. D. Reames
6. Yuming Wang
7. C. Farrugia
8. C. Cohen

Citations in the corpus

• Solar flares, coronal mass ejections and solar energetic particle event characteristics (2016, methodology): “The validity of the VDA method has been an item of active research by several authors (Lintunen & Vainio 2004; Sáiz et al. 2005; Rouillard et al. 2012; Vainio et al. 2013), with the VDA method typically used to estimate the SRT of SEP events (Lario et al.”
• The Two Sources of Solar Energetic Particles (2012, methodology): “…the following: 1) reduced shock speed on the flanks when a single shock or CME speed was assumed or 2) the shock actually expands to strike field lines at higher altitudes on the flanks, as, for example, shown by the STEREO simulations in the left panels of Figure 3.4 (Rouillard et al. 2011, 2012).”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “Studies on Moreton and EUV waves are still unresolved and cannot fully rule out coronal waves as SEP driving agent (against: Bothmer et al., 1997, Krucker et al., 1999, Miteva et al., 2014; pro: Malandraki et al., 2009, Rouillard et al., 2012).”
• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…spatio–temporal correlation between the releases of SEPs and the arrivals of EIT waves at their source regions connected by open magnetic-field lines to observers at multiple viewpoints (e.g. Kozarev et al., 2011; Rouillard et al., 2011, 2012; Nitta, 2012; Park et al., 2013; Miteva et al., 2014).”
• The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event (2012, background): “2 right) may also influence the coronal particle propagation as suggested by Rouillard et al. (2012).”
• > 25 MeV Proton Events Observed by the High Energy Telescopes on the STEREO A and B Spacecraft and/or at Earth During the First ∼ Seven Years of the STEREO Mission (2014, background): “Rouillard et al. (2012) noted that an EUV wave tracked the laterally-expanding flank of the 21 March 2011 CME, moving parallel to the surface of the Sun at ∼ 450 km s−1.”