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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 14.

Neutron-energy dependence of the decay factors identified in Equation (1) for several distances d from the flare site. The gray band identifies the 30–100 keV suprathermal energy range. Panel (a) shows the neutron survival probability and the differential decay probability. Panel (b) shows the product of these two probabilities.

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