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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 4.

Solid curves are angle-dependent neutron spectra escaping from the Sun (prior to any neutron decay) for a downward-isotropic interacting-ion angular distribution (δ = 0 and ﹩\lambda \to \infty ﹩), shown for several direction angles ψn. The dashed curve is the angle-integrated neutron spectrum at production within the solar atmosphere. The gray band identifies the 30–100 keV energy range.

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