Computer Science
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jqsrt.100..220l&link_type=abstract
Journal of Quantitative Spectroscopy and Radiative Transfer, Volume 100, Issue 1-3, p. 220-236.
Computer Science
35
Scientific paper
The present study intends to interpret some of the characteristic features of the light scattered by cometary dust, such as phase angle and wavelength dependence of its polarization, through simulations using Ballistic Cluster-Cluster Aggregation (BCCA) or Ballistic Particle-Cluster Aggregation (BPCA) aggregates of up to 128 sub-micron sized grains (spherical and spheroidal with a possible size distribution) of various composition (silicates, organics, silicates core with organics mantle). The dependence of the linear polarization with the size parameter is shown to depend highly on the size and composition of the constitutive grains. Internal interactions induced by shape or orientation averaging of the grains may lessen this dependence, leading to results comparable to those observed on cometary dust for fluffy aggregates of grains with a size parameter in the 1.3 1.8 range. A size distribution of realistically shaped particles (aggregates of spheroids and larger spheroids) following a power law size distribution with a power index of -3, the smallest grains radius by 0.03 0.2μm and the largest spheroids effective radius by 20μm, gives a very good fit to the Hale-Bopp observed phase curves. The best silicates organics ratio ranges from about 50 75% organics and 25 50% silicates in volume considering the eventual presence of core-mantle grains.
Lasue Jeremie
Levasseur-Regourd Anny-Chantal
No associations
LandOfFree
Porous irregular aggregates of sub-micron sized grains to reproduce cometary dust light scattering observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Porous irregular aggregates of sub-micron sized grains to reproduce cometary dust light scattering observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Porous irregular aggregates of sub-micron sized grains to reproduce cometary dust light scattering observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1794400