LONGITUDINAL AND RADIAL DEPENDENCE OF SOLAR ENERGETIC PARTICLE PEAK INTENSITIES: STEREO, ACE, SOHO, GOES, AND MESSENGER OBSERVATIONS

By D. Lario, À. Aran, R. Gómez-Herrero, N. Dresing, B. Heber, G. Ho, R. Decker, E. Roelof. 2013

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> 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, methodology): “(Note that this is the opposite convention to that used by Lario et al., 2013 in their study of SEP longitudinal intensity dependence that includes some of the same events.)”
Solar flares, coronal mass ejections and solar energetic particle event characteristics (2016, background): “Further work should focus on the effect of DU on the derived SEP flux (Lario et al. 2013), given the fact that, two critical DU at about 30 and 50 , delimiting three zones for which the importance of the longitudinal gradient is different from one another greatly affect the flux variability of SEP e”
History and development of coronal mass ejections as a key player in solar terrestrial relationship (2016, background): “Multiple views also helped recognize many SEP events that are observed all around the Sun (see e.g., Dresing et al. 2012; Lario et al. 2013) providing opportunities to test the CME origin and heliospheric propagation of energetic particles.”