Figure 3 from Neutron-decay Protons from Solar Flares as Seed Particles for CME-shock Acceleration in the Inner Heliosphere

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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 3.

Angle-integrated energy spectra of neutrons at production (before transport through the solar atmosphere) for ion spectral indexes Γ of 2, 4, and 6. The gray band identifies the 30–100 keV energy range. The calculations are normalized to N_p(>30 MeV) = 1.

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