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An overview of our present efforts at the Bartol Research Institute in modelling the large-scale 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.
Keyword:
interstellar neutrals
numerical modelling
solar wind
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7.4
论文数:
4.2K
被引数:
1.8W
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