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Fig. 2.


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From top to bottom: (a) relative count rate increases of selected neutron monitor stations located in proximity of the analysed flight route (cf. Fig. 1); (b) calculated effective dose rates from galactic cosmic rays (GCR) and solar energetic particles (SEP) for the different scenarios; (c) altitude profiles of the different flight scenarios; (d) effective cut-off rigidities Rc of the different scenarios.

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