Physics
Scientific paper
Sep 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9815157b&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A9, p. 15,157-15,163.
Physics
270
Flow Distribution, Interstellar Matter, Magnetohydrodynamic Flow, Plasma Composition, Plasma-Particle Interactions, Solar Wind, Hydrogen Atoms, Iterative Solution, Mathematical Models, Monte Carlo Method
Scientific paper
Results are presented for the self-consistent problem solution of a single set of undisturbed solar wind and local interstellar medium parameters, encompassing calculations of the structure of the upwind as well as wake regions of the flow. The geometrical pattern of the flow, and the bulk velocity and number densities of the H atoms and plasma components are derived and analyzed as a function of solar diatance for different polar angle values. It is noted that the effect of the penetration of the solar wind by the H atoms is a vanishing of the complex flow structure and of the supersonic regions betwen the heliopause and the termination shock in the downwind region.
Baranov Vladimir B.
Malama Yu. G.
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