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Figure 7

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Martian surface flux of proton, electron & positron, muon and pion at Gale Crater from 19 August 2012 to 17 February 2013, given by ARAMIS and compared to measurements and other models with FTFP_INCLXX_HP. For protons, solid lines represent cone-viewed downward spectra, while dashed lines represent direction-averaged spectra.

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