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Figure 3 | Earth, Planets and Space

Figure 3

From: Performance of the SciBar cosmic ray telescope (SciCRT) toward the detection of high-energy solar neutrons in solar cycle 24

Figure 3

Detection efficiency for neutrons. Relationship between the energy of incident neutrons and the estimated effective area injected with five different zenith angles. The azimuth angle and injected direction are chosen randomly for each event. The pink plots show the effective area of vertical injection of particles on the Mexico SNT calculated by the detection efficiency (González et al. 2010) and detector size (4 m2) (Nagai et al. 2014).

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