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Date: 2018-03-18 17:08:07 | ACE News 197 – March 19, 2018 Can Solar Flare Neutron-Decay Protons Provide a Seed Population for CME Shock Acceleration? Fig. 1: Neutron-decay proton densities for the indicated conditions and for 10° (a) and 45° (bAdd to Reading ListSource URL: www.srl.caltech.eduDownload Document from Source WebsiteFile Size: 993,01 KBShare Document on Facebook |