Revised GLE database: Fluences of solar energetic particles as measured by the neutron-monitor network since 1956

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Fig. 4.

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Dependence of the χ² value on the MER spectral parameters (Eq. (5)) for GLE 38 shown in Fig. 3. The best-fit values () are shown with the red stars. The horizontal dashed blue line corresponds to , and the vertical blue arrows denote the 68% bounds for the parameter values.

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