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• W2170940539 abstract "The radiation protection is one of the two NASA highest concerns priorities [1]. In view of manned missions targeted to Mars [2], for which radiation exposure is one of the greatest challenges [3], it is fundamental to determine particle fluxes and doses at any time and at any location and elevation on and around Mars [4]. With this goal in mind, models of radiation environment induced by Galactic Cosmic Rays (GCR) and Solar Particle Events (SPE) on Mars and Phobos have been developed [5]. The work is de-scribed [6] as incoming cosmic ray [7-9] and solar events [5-6] primary particles rescaled for Mars condi-tions then transported through the atmosphere down to the surface, with topography and backscattering taken into account, then through the subsurface layers, with volatile content and backscattering taken into account, eventually again through the atmosphere, and interact-ing with some targets described as material layers. Models have been developed for the surface of the satellites Phobos, as well as for the cruise phase. These results for Mars and Phobos Radiation Environment have been obtained in the framework of the LIULIN-PHOBOS investigation that will be onboard the PHOBOS-GRUNT mission by the Russian Space Agency RKA. The LIULIN-PHOBOS investigation is described in another LPSC 2009 paper by Ts. Dachev." @default.
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• W2170940539 date "2009-03-01" @default.
• W2170940539 modified "2023-09-25" @default.
• W2170940539 title "Models for the Radiation Environment of Planet Mars and of Its Moon Phobos" @default.
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• W2170940539 hasPublicationYear "2009" @default.
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