Dust emission studies in Halley's inner coma: an approach to modelling the nucleus emission characteristics

Details Dust emission studies in Halley's inner coma: an approach to modelling the nucleus emission characteristics Dust emission studies in Halley's inner coma: an approach to modelling the nucleus emission characteristics

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250b.201p&link_type=abstract

In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus p 201-206 (SEE N

Mathematics

Comet Nuclei, Cosmic Dust, Halley'S Comet, Mass Distribution, Giotto Mission, Mathematical Models, Vega Project

Scientific paper

Using a modelling process for the dynamics of particulates emitted from Halley at distances much smaller than the apex of the dust envelope, fluxes measured by Giotto DIDSY and Vega 2 are traced back to Halleycentric nucleus co-ordinates to yield a unified comparison of the two data sources. Mass distribution indices are interrelated, and, of particular significance, properties of the angular source distribution of Halley relative to the sub-solar emission point are examined. Variability of the nucleus emission rate is discussed.

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