Figure 9 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 9.

Distance r from the center of the Sun to the point p on the magnetic field line as a function of distance s along the field line for V_SW = 450 km s⁻¹ and with the field-line footpoint located on the solar equator (θ_B = 0°). The dash–dot line is s = r.

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