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Simulation of ICE-Giacobini-Zinner and VEGA/GIOTTO-Halley encounters
Authors:Th Roatsch  K Sauer  K Baumgärtel
Institution:(1) Institut für Kosmosforschung der Akademie der Wissenschaften der DDR, Berlin, D.D.R.
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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