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We present a new model of the heliospheric interface - the region of thesolar wind interaction with the local interstellar medium. This new modelperforms a multi-component treatment of charged particles in the heliosphere.All charged particles are divided into several co-moving types. The coldesttype, with parameters typical of original solar wind protons, is considered inthe framework of fluid approximation. The hot pickup proton components createdfrom interstellar H atoms and heliospheric ENAs by charge exchange, electronimpact ionization and photoionization are treated kinetically. The chargedcomponents are considered self-consistently with interstellar H atoms, whichare described kinetically as well. To solve the kinetic equation for H atoms weuse the Monte Carlo method with splitting of trajectories, which allows us 1)to reduce statistical uncertainties allowing correct interpretation ofobservational data, 2) to separate all H atoms in the heliosphere into severalpopulations depending on the place of their birth and on the type of parentprotons.Comment: A&A accepte

Modeling of the heliospheric interface: multi-component nature of the heliospheric plasma