Statistics – Computation
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..654z&link_type=abstract
Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 654
Statistics
Computation
2
Solar Wind Plasma, Sources Of Solar Wind, Interplanetary Dust And Gas, Hydrodynamics, Planetary Bow Shocks, Interplanetary Shocks
Scientific paper
The interaction of the solar wind with the local interstellar medium (LISM) is investigated on the basis of a time-dependent 2D model in which the plasma is described hydrodynamically and the interstellar neutrals by a Boltzmann equation modified by charge exchange. This computationally intensive calculation yields results qualitatively in accord with the simpler Pauls et al. [1995] 2-fluid model, thus validating a careful hydrodynamic approach. The results of simulations for a 2-shock model and a 1-shock model are described and compared and some observationally distinguishable characteristics are identified.
Hall Doyle T.
Pauls Louis H.
Williams Lance Lee
Zank Gary P.
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