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Physical processes in the tail of the solar wind interaction region with thepartially ionized local interstellar medium are investigated in a framework ofthe self-consistent kinetic-gas dynamic model. It is shown that the chargeexchange process of the hydrogen atoms with the plasma protons results insuppression of the gas dynamic instabilities and disappearance the contactdiscontinuity at sufficiently (~3000 AU) large distances from the Sun. Thesolar wind plasma temperature decreases and, ultimately, the parameters of theplasma and hydrogen atoms approach to the corresponding parameters of theunperturbed interstellar medium at large heliocentric distances.Comment: first version, final version is published in Astronomy Letters vol.29  N.1, pp.58-63, 200

A model for the tail region of the heliospheric interface