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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 13.

Time-integrated neutron-decay proton energy spectra at various positions s along the field line for a flare and a field line footpoint located on the equator (θf = 0° and θB = 0°). Panel (a) is for a footpoint longitude of ϕB = 45°, and panel (b) is for ϕB = 10°. The gray band identifies the 30–100 keV energy range.

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