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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 11.

Angle ψn (the angle between the neutron direction and the normal to the solar surface at the flare site) as a function of distance s along the magnetic field line for several values of the footpoint latitude θB. Panel (a) is for a field-line footpoint longitude ϕB = 45° and panel (b) is for ϕB = 10°.

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