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dc.contributor.authorMaci, D.
dc.contributor.authorKeppens, R.
dc.contributor.authorBacchini, F.
dc.date2025
dc.date.accessioned2026-01-02T10:31:00Z
dc.date.available2026-01-02T10:31:00Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/14517
dc.descriptionUnderstanding the effect of turbulent magnetic fluctuations on the transport of energetic particles is a fundamental, still unanswered problem in astrophysics. In this paper we present a novel framework aimed at the study of cosmic rays transport and diffusion on the basis of test particle simulation in synthetic turbulent realizations. In particular, we make use of the BxC toolkit, integrating its output within the MPI-AMRVAC framework. We show that the two codes are successfully interfaced, paving the way for an extensive parameter study that could give insight into the role of turbulence in particle diffusion and scattering.
dc.languageeng
dc.titleToward applications of the BxC toolkit
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleJournal of Physics: Conference Series, ASTRONUM 2024 - the 16th International Conference on Numerical Modeling of Space Plasma Flows, La Rochelle, France, 1-5 July, 2024
dc.source.volume2997
dc.source.pageA012003
Orfeo.peerreviewedYes
dc.identifier.doi10.1088/1742-6596/2997/1/012003
dc.identifier.url


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