Database of optical properties of cosmic dust analogues (DOP)
| dc.creator | Il'in, V. B. | |
| dc.creator | Voshchinnikov, N. V. | |
| dc.creator | Babenko, V. A. | |
| dc.creator | Beletsky, S. A. | |
| dc.creator | Henning, Th. | |
| dc.creator | Jaeger, C. | |
| dc.creator | Khlebtsov, N. G. | |
| dc.creator | Litvinov, P. V. | |
| dc.creator | Mutschke, H. | |
| dc.creator | Tishkovets, V. P. | |
| dc.creator | Waters, L. B. F. M. | |
| dc.date | 2003-08-11 | |
| dc.date.accessioned | 2026-07-07T02:09:12Z | |
| dc.date.available | 2026-07-07T02:09:12Z | |
| dc.description | 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. | |
| dc.description | 6 pages with 4 figures, submitted to A&A | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0308175 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0308175 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6345 | |
| dc.subject | Astrophysics | |
| dc.title | Database of optical properties of cosmic dust analogues (DOP) | |
| dc.type | text |