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.
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Zank, G.P., Pauls, H.L. Modelling the heliosphere. Space Sci Rev 78, 95–106 (1996). https://doi.org/10.1007/BF00170796
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DOI: https://doi.org/10.1007/BF00170796