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Database of Optical Properties next up previous
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Database of Optical Properties

In astrophysics, the optical constants mainly are used to calculate the optical properties of scatterers, i.e. cross-sections, scattering matrix, etc. For many applications, it is necessary to understand general trends in the data. This understanding often can be gained from consideration of results obtained by simplified scattering models. Optical properties derived from such models have been discussed in some books (see, e.g., [2,3]) and in principle can be calculated by using various light-scattering tools which are freely available via the internet [4]. Nevertheless, there is a definite necessity of a WWW database devoted to systematic consideration of the optical properties of various model scatterers and related topics. As of this writing, our database will include: The work on all the parts of the DOP is either in progress or has been finished. It is undertaken by several persons from different institutes of former Soviet Union countries under support of an INTAS grant. The DOP will be (partly) available via the Internet [5] upon its completion scheduled at the end of 2002. Because of the large volume due to the graphics library, the whole database may be available only on CDs.
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Next: Examples of data contained Up: Electronic database Previous: Future plans
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