Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999astl...25..825b&link_type=abstract
Astronomy Letters, Volume 25, Issue 12, December 1999, pp.825-832
Astronomy and Astrophysics
Astronomy
3
Scientific paper
The problem of the magnetic-field distribution at the heliospheric interface is solved in the kinematic approximation for various densities of the charged and neutral interstellar-medium components. In particular, it is shown that an increase in the density of the two components causes a reduction in the influence of the interstellar magnetic field, while the influence of the interplanetary magnetic field is mainly determined by a dimensionless parameter, the ratio of these densities. The distributions of the gas-dynamical quantities which are needed to determine the structure of the magnetic field at the heliospheric interface and to estimate its possible influence were taken from the kinetic-gas-dynamical model of Baranov and Malama (1993, 1995, 1996).
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