Simulation of ICE-Giacobini-Zinner and VEGA/GIOTTO-Halley encounters |
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| Authors: | Th. Roatsch K. Sauer K. Baumgärtel |
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| Affiliation: | (1) Institut für Kosmosforschung der Akademie der Wissenschaften der DDR, Berlin, D.D.R. |
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| Abstract: | The formation of a weak shock at the interaction of the solar wind with the cometary neutral gas is confirmed in a non-stationary gasdynamic model. No shocks will be detectable along the ICE path and if the VEGA/GIOTTO spacecraft enter the cometary atmosphere. A shock can only be expected at an exit from the Halley atmosphere. |
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