Modelling Halley's dust coma from a 3D+t dusty gasdynamic model

Details Modelling Halley's dust coma from a 3D+t dusty gasdynamic model Modelling Halley's dust coma from a 3D+t dusty gasdynamic model

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....5480f&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #5480

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The cometary activity steady-state 3D physical model of Rodionov et al., Planetary and Space Sciences, 50, 983 - 1024 (2002) model has been successfully applied to account for the near-nucleus dust features observed from the VEGA and Giotto cameras, and for the in-situ GIOTTO dust detections. An upgraded version of this model has been recently developed: it is tridimensional as previously, and, in addition, time-dependent. This allows an exact self-consistent computation of the whole dust coma structure, moreover fitting the VEGA in-situ dust detector results. This presentation shows the computed time-dependent near-nucleus dust distribution, and the resulting fits to the in-situ detectors.

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