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It is extremely important to understand and model the Martian radiationenvironment in preparation for future human missions to Mars, especially duringextreme and elevated conditions such as an intense solar energetic particle(SEP) event. Such events may enhance the radiation level drastically and shouldbe forecasted as soon as possible to prevent severe damage to humans andequipment. Besides, the omnipresent galactic cosmic rays (GCRs) also contributesignificantly to the radiation in space and on the surface of Mars and maycause long-term damages to current and future missions. Based on GEANT4 MonteCarlo simulations with the Martian atmospheric and regolith environment setup,we have calculated and obtained some ready-to-go functions which can be used toquickly convert any given SEP or GCR proton/helium ion spectra to the radiationdose on the surface of Mars and also at different depth of the atmosphere. Weimplement these functions to the RADMAREE tool under the Europlanet projectwhich can be easily accessed by the public.

Ready functions for calculating the Martian radiation environment