Aggregates model to describe light scattering by cometary dust

Details Aggregates model to describe light scattering by cometary dust Aggregates model to describe light scattering by cometary dust

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..161l&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

We study the light scattered by cometary dust particles, more precisely Ballistic-Cluster-Cluster (BCCA) or Particle-Cluster (BPCA) aggregates of up to 128 sub-micron sized silicates or organics grains (spherical and spheroidal). A mixture of 40% to 70% organics and silicates (respectively 60% to 30%) provides the best fit to comet Hale-Bopp dependence of linear polarization, P, with the wavelength, λ, and the phase angle, α.

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