The interpretation of the mid-infrared spectrum of comets: effects of particle non-sphericity

Details The interpretation of the mid-infrared spectrum of comets: effects of particle non-sphericity The interpretation of the mid-infrared spectrum of comets: effects of particle non-sphericity

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003elsn.conf..239m&link_type=abstract

In: Electromagnetic and Light Scattering - Theory and Applications VII, Editor Thomas Wriedt, ISBN 3-88722-579-1, 2003, p. 239-2

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Applications

Spectrum, Hale-Bopp, Dust

Scientific paper

We present an analysis of comet Hale-Bopp spectrum in the mid-infrared as obtained from the Infrared Space Observatory (ISO) [1]. While it is possible to reproduce the spectrum by a combination of silicates and carbon rich spherical particles, a proper interpretation should take into account the particle non-sphericity, and some calculations of the absorption efficiency for non-spherical particles are provided in comparison with the observed spectrum.

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