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Fig. 9


Propagated spectra in the absence of magnetic turbulence for models (left column) and (right column) neglecting and accounting for gyromotion effects (upper and lower row, respectively). Blue solid and red dashed lines show the attenuated proton and secondary electron spectra, respectively, at increasing depth in the cloud labelled by values of the column density along the line of sight, log 10 [ Nlos(H2)/cm-2 ].

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