Figure 1 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 1.

Differential intensity of protons at 1 au measured with SWICS and ULEIS on ACE during quiet times in 2007 (taken from Figure 3 of Gloeckler et al. 2008). The components of the solar wind are noted. The gray band identifies the 30–100 keV energy range.

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