Modelling the 5 30 Μm spectrum of Comet Halley

Details Modelling the 5 30 Μm spectrum of Comet Halley Modelling the 5 30 Μm spectrum of Comet Halley

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988em%26p...43..145w&link_type=abstract

Earth, Moon and Planets, Volume 43, Issue 2, pp.145-153

Computer Science

2

Scientific paper

The 5 - 30 μm spectrum of Comet P/Halley is modelled for various grain compositions on the basis of an observationally determined distribution of grain sizes. The authors compute the distribution function of grain temperatures and fluxes arising from (1) a mineral grain model, and (2) an organic grain model comprised of a diatom/POM mixture. The organic/POM model yields excellent accord with the cometary observations.

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