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Fig. 2.


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Primary GCR spectra, exemplarily for hydrogen (Z = 1), helium (Z = 2), carbon (Z = 6), and iron (Z = 26), for the time between August 2012 and January 2013 as described by the DLR (Matthiä et al. 2013) and Badhwar/O’Neill 2010 (BO-10) (O’Neill 2010) models. Calculations were performed taking into account all primary nuclei from hydrogen to iron.

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