Abstract—
It is believed that microscopic life is possible in the subglacial ocean of Europa, a satellite of Jupiter. However, Jupiter’s radiation belts make it difficult to detect it on the surface or at shallow depths. Using numerical simulations, we investigated the influence of the inclination of the magnetic dipole of Jupiter, the Alfvén wings, and the induced field of Europa on the dynamics of electrons near the satellite of Jupiter, which made it possible to refine the map of radiation doses on Europa’s surface, obtained earlier in the approximation of the guiding center.
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Funding
The authors are grateful to the Government of the Russian Federation and the Ministry of Higher Education and Science of the Russian Federation for the support of the following works under the grant 075-15-2020-780 (N13.1902.21.0039): 1) building a model of the dynamics of electrons near Europa, 2) calculating radiation doses on the surface of Europa under a layer of water of various thicknesses, 3) building a map of the distribution of radiation doses on the surface of Europa. Research by E.P. Popova was supported by the Russian Science Foundation under the grant 17-11-01052. Within the framework of the Russian Science Foundation grant 17-11-01052, E.P. Popova formulated the problem and magnetic field models were proposed.
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Tsareva, O.O., Popova, E.P., Popov, V.Y. et al. Modeling the Dose Distribution of Electron Radiation on the Surface of Jupiter’s Satellite Europa for Different Magnetic Field Models. Sol Syst Res 55, 335–340 (2021). https://doi.org/10.1134/S0038094621040109
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DOI: https://doi.org/10.1134/S0038094621040109