Implementation and validation of the GEANT4/AtRIS code to model the radiation environment at Mars | Journal of Space Weather and Space Climate

Open Access

Fig. 12

Martian surface spectra of H (panel a) and He (panel b) isotopes induced by primary GCR proton and ⁴He particles modeled via four different physics lists (Table 1). The spectra are averaged within 36° of downward zenith angle corresponding to the RAD view cone. (a) Input: GCR H + ⁴He, output: downward H isotopes, (b) input: GCR H + ⁴He, output: downward He isotopes.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.