Self-consistent hybrid simulations of the interaction of the heliosphere with the local interstellar medium

Details Self-consistent hybrid simulations of the interaction of the heliosphere with the local interstellar medium Self-consistent hybrid simulations of the interaction of the heliosphere with the local interstellar medium

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..819m&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 819-822 (1999).

Physics

2

Interplanetary Physics, Atomic, Molecular, And Chemical, And Grain Processes

Scientific paper

A hydrodynamic plasma simulation of the ionized component of the global heliosphere has been coupled to a nonstationary Boltzmann particle-mesh method which describes the neutral hydrogen present in the same region. This coupling is a numerical model of the physical charge-exchange process through which the two particle species interact. Numerical self-consistency is achieved by iterating the distributions of the two particle species between the two numerical schemes until a steady state is achieved. This approach will contribute to the understanding of the solar wind-LISM interaction.

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