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Database of optical properties of cosmic dust analogues (DOP)

V. B. Il'in·N. V. Voshchinnikov·V. A. Babenko·S. A. Beletsky·Th. Henning·C. Jaeger·N. G. Khlebtsov·P. V. Litvinov·H. Mutschke·V. P. Tishkovets·L. B. F. M. Waters
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Abstract

We present a database containing information on different aspects of calculation and usage of the optical properties of small non-spherical particles -- cosmic dust analogues. The main parts of the DOP are a review of available methods of the light scattering theory, collection of light scattering codes, special computational tools, a graphic library of the optical properties (efficiencies, albedo, asymmetry factors, etc.), a database of the optical constants for astronomy, a bibliographic database of light scattering works, and links to related Internet resources. The general purpose of the DOP having the address http://www.astro.spbu.ru/DOP is twofold -- to help scientists to apply the light scattering theory in astronomy and to give students and beginners a possibility quickly to get necessary knowledge on the subject.

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V. B. Il'in, N. V. Voshchinnikov, V. A. Babenko, S. A. Beletsky, Th. Henning, C. Jaeger, N. G. Khlebtsov, P. V. Litvinov, H. Mutschke, V. P. Tishkovets, L. B. F. M. Waters. 2003-08-11. Database of optical properties of cosmic dust analogues (DOP). https://arxiv.org/abs/astro-ph/0308175

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