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Neutron-decay Protons from Solar Flares as Seed Particles for CME-shock Acceleration in the Inner Heliosphere

  • Authors: Ronald J. Murphy, and Yuan-Kuen Ko

2017 The Astrophysical Journal 846 53.

  • Provider: AAS Journals

Caption: Figure 12.

Neutron arrival time at the field line as a function of distance along the field line s for various neutron energies En (keV). The neutron arrival time corresponds to the production time of decay protons from those neutrons that decay there. The gray band identifies the 30–100 keV energy range.

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