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Scattering matrices and reflectance spectra of forsterite particles with different size distributions
Authors:H Volten  O Muoz  JR Brucato  JW Hovenier  L Colangeli  LBFM Waters  WJ van der Zande
Institution:

aAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands

bInstituto de Astrofísica de Andalucía, CSIC, Camino Bajo de Huétor 50, Granada 18008, Spain

cINAF - Osservatorio Astronomico di Capodimonte, via Moiariello 16, 80131 Napoli, Italy

dInstituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200B, B-3001 Heverlee, België

eInstitute for Molecules and Materials, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, The Netherlands

Abstract:We present measurements of the complete scattering matrix as a function of the scattering angle of three different samples of forsterite particles in random orientation at a wavelength of 632.8 nm. The three samples were prepared so that three different size distributions were obtained. The composition and reflection spectra of the three samples have been experimentally determined. The results indicate that the elements of the scattering matrix are affected in a different way by the size differences. Since light scattering by comets is probably caused by particles similar to our forsterite particles, the results potentially contain information on the size of the cometary particles.
Keywords:Scattering  Polarization  Comets  Dust  Forsterite
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