Space Science Reviews

, Volume 78, Issue 1–2, pp 95–106 | Cite as

Modelling the heliosphere

The Heliosphere

Abstract

An overview of our present efforts at the Bartol Research Institute in modelling the largescale interaction of the solar wind with the local interstellar medium is presented. Particular stress is placed on the self-consistent inclusion of neutral hydrogen in the models and both 2D and 3D structure is discussed. Observational implications are noted.

Key words

interstellar neutrals numerical modelling solar wind 
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Copyright information

© Kluwer Academic Publishers 1996

Authors and Affiliations

  1. 1.Bartol Research InstituteUniversity of DelawareUSA

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