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- W1979863022 abstract "Abstract Modelling of the pick-up ion fluxes for the water group (H2O+, O+, OH+) far upstream of comet Halley during the Giotto fly-by is continued with additional refinements over the earlier attempts. These are: inclusion of the contributions to O from the dissociations of the minor cometary components CO and CO2; using the in situ measured magnetic field and solar wind data to determine the direction of integration for the ion flux calculation. As in the previous works, the neutral densities that feed the ions are calculated with the Kepler trajectory model. Comparisons of the model results with the ions measured by EPONA on board Giotto demonstrate agreement in general for relative changes, at least on the inbound leg. This implies that much of the structure seen in the EPONA data is a result of changing solar wind conditions." @default.
- W1979863022 created "2016-06-24" @default.
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- W1979863022 date "1992-08-01" @default.
- W1979863022 modified "2023-09-23" @default.
- W1979863022 title "Cometary water group ion fluxes calculated along the Giotto trajectory under observed solar wind conditions" @default.
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- W1979863022 doi "https://doi.org/10.1016/0273-1177(92)90407-o" @default.
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