Figure 8 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 8.

Illustration of various geometrical variables for the special case of the magnetic field line in the x–y plane (θ_B = 0°) and the flare on the equator (θ_f = 0°)). The view is looking down on the x–y (equatorial) plane.

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