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Home All issues A&A, 472 1 (2007) 283-286 Article references

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Cited article:

Spectra and Anisotropy of Solar Energetic Protons During GLE #65 on 28 October, 2003 and GLE #66 on 29 October, 2003

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Statistical Research on the Longitudinal Distribution of Detected Properties of Solar Energetic Particles

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Small, Low-energy, Dispersive Solar Energetic Particle Events Observed by Parker Solar Probe

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Is the enhancement of type II radio bursts during CME interactions related to the associated solar energetic particle event?

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Research in Astronomy and Astrophysics 19 (1) 005 (2019)
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Dependence ofE≥ 100 MeV protons on the associated flares and CMEs

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Research in Astronomy and Astrophysics 17 (7) 073 (2017)
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ARE THERE TWO DISTINCT SOLAR ENERGETIC PARTICLE RELEASES IN THE 2012 MAY 17 GROUND LEVEL ENHANCEMENT EVENT?

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The Astrophysical Journal 818 (2) 169 (2016)
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Geoeffectiveness of the coronal mass ejections associated with solar proton events

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ELECTRON AND PROTON ACCELERATION DURING THE FIRST GROUND LEVEL ENHANCEMENT EVENT OF SOLAR CYCLE 24

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The Astrophysical Journal 735 (2) 113 (2011)
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SUNSPOT ROTATION, FLARE ENERGETICS, AND FLUX ROPE HELICITY: THE HALLOWEEN FLARE ON 2003 OCTOBER 28

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The Astrophysical Journal 722 (2) 1539 (2010)
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The X17.2 flare occurred in NOAA 10486: an example of filament destabilization caused by a domino effect

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Solar source of energetic particles in interplanetary space during the 2006 December 13 event

C. Li, Y. Dai, J.-C. Vial, et al.
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An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles

V. V. Grechnev, V. G. Kurt, I. M. Chertok, et al.
Solar Physics 252 (1) 149 (2008)
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Solar release time of solar energetic particles and associated acceleration source in corona

GuiMing Le, YuHua Tang and YanBen Han
Chinese Science Bulletin 53 (2) 161 (2008)
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Radio Submillimeter and γ‐Ray Observations of the 2003 October 28 Solar Flare

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The Astrophysical Journal 678 (1) 509 (2008)
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