Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ioch.rept...22h&link_type=abstract
In NASA, Washington, Infrared Observations of Comets Halley and Wilson and Properties of the Grains p 22-49 (SEE N89-13330 04-89
Astronomy and Astrophysics
Astronomy
45
Chemical Composition, Cosmic Dust, Emission Spectra, Halley'S Comet, Light Scattering, Optical Properties, Grain Size, Infrared Astronomy, Infrared Spectra, Optical Polarization, Particle Size Distribution, Silicates, Solar Flux, Spectral Energy Distribution
Scientific paper
The optical properties of small grains provide the link between the infrared observations presented in Chapter 1 and the dust composition described in Chapter 3. In this session, the optical properties were discussed from the viewpoint of modeling the emission from the dust coma and the scattering in order to draw inference about the dust size distribution and composition. The optical properties are applied to the analysis of the infrared data in several ways, and these different uses should be kept in mind when judging the validity of the methods for applying optical constants to real grains.
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