|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.astro.spbu.ru/DOP/5-OPTC/DESCRIPT/index.html
Дата изменения: Fri Nov 19 12:07:05 2010 Дата индексирования: Mon Oct 1 23:58:59 2012 Кодировка: Поисковые слова: п п п п п п п п п п р п р п п р п р п п р п р п п р п |
WWW database of optical constants for astronomyTh. Henning1, V.B. Il'in2, N.A. Krivova2, B. Michel1, N.V. Voshchinnikov2 1 Astrophysical Institute and University Observatory,
Friedrich Schiller University,
Schillergaesschen 3, D-07745 Jena, Germany Published in Astron. Astrophys. Suppl. 136, 405 (1999)
1. IntroductionThe optical constants of materials - refractive indices or dielectric permittivities - are widely used in astrophysics. They are input parameters required for any simulations of the light scattering by dust grains and the calculations of radiative transfer in dusty media (galaxies, interstellar clouds, circumstellar shells, protoplanetary disks, atmospheres of brown dwarfs). Since the 60's the volume of the data has been permanently growing and presently it is difficult to overlook the results obtained within about 40 years. We attempted to collect and classify the data available and to create a place in the Internet for further accumulation of such data.2. The databaseThe main topics of the database are the optical constants of materials involved in astronomical calculations. These materials are:
2.1. ReferencesThe database contains about 500 references to the papers, books, dissertations where the refractive indices, reflectance, transmittance, mass absorption coefficient, and so on were derived. Most of the papers were published in the time interval from the 60's till 1998.2.2. DataWe have started filling the database with the data available for us. They are the optical constants obtained in the laboratory of Astrophysical Institute of Friedrich Schiller University (Jena) as well as the data derived in the Soviet Union and some often used freely accessible data.It should be noted that the Jena data were intended especially for astronomical applications. They cover a wide spectral range, show the dependence on important parameters: Fe/Mg ratio, temperature, etc. Besides, well prepared samples and sophisticated control were used in these measurements (see, e.g., Jaeger et al., 1994; Jaeger et al., 1998; Schnaiter et al., 1998). Several papers on the optical constants of the materials under consideration were published in former Soviet Union journals (see Zolotarev et al., 1984 for a review). As these journals are not easily accessible, we scanned the data tables/figures in the papers printed before 1974 (when the Soviet Union joined the international copyright agreement) and put them in our database. The data we included are presented in their initial format (table or figure) and in our standard tabular format. In some cases we also give plots of the refractive index vs wavelength and dielectric permittivity vs energy dependences and an information on how the data were obtained, what equipment was used and what samples were considered. The service codes of the database allow to transfer the data from our standard format to a desirable form (refractive index/dielectric permittivity vs wavelength/wavenumber/energy table with numbers of any format). Our light scattering codes based on Mie theory and Separation of Variables Method for spheroids give the possibility to transform the data into cross-sections, emissivity and so on. 2.3. Related topicsReferences to some useful books and reviews on the subject (e.g. the classical handbooks by Palik, 1985, 1991) and links to Internet collections of optical data files and personal WWW pages with related software were also placed in the database.First of all, among these Internet resources one should mention the WWW database of the optical constants in the X-ray domain created at the Lawrence Berkeley National Laboratory ( http://www-cxro.lbl.gov/optical_cons tants), and the collections of the data files obtained for a very large number of ice mixtures at the Leiden University (http://www.strw.leidenuniv.nl/~lab) and for amorphous carbon by V. Zubko (http://physics.technion.ac.il/~zubko/nk.html). There are also useful tools for the Kramers-Kronig analysis and Effective Medium Theory available in the World Wide Web. Many light scattering codes have been developed and there are two general lists of such codes in the Internet. Besides links to these lists, we also give direct links to personal WWW pages where one can find most popular codes to simulate the electromagnetic radiation scattering by spheres (Mie theory), spheroids (Separation of Variables Method), axisymmetric particles (T-matrix Method), irregular-shaped particles (Discrete Dipole Approximation) and others. 2.4. Some detailsAnyone can freely access the database - its Internet address is http://www.astro.spbu.ru/JPDOC/entry.html (server in St. Petersburg) or http://www.astro.uni-jena.de/Users/database/entry.html (server in Jena). First, one will arrive at a welcome WWW page with a short description of the database and a link to the database homepage. The latter includes our list of the material groups (silicates, oxides and so on) and a description of related topics (Internet resources, books, etc).Each group of materials has its own page. It contains a table whose columns show: the state of material (amorphous, crystalline, glassy), the quantity measured or calculated (refractive index, reflectance, etc), the form of the data (table, figure), the considered wavelength range (in microns), and reference to the paper. When the data in a paper were available we created a corresponding WWW page and supplied the table with a link to the page. Such pages can contain links to data and graphic files, information about the paper (e.g. its ADS abstract), a description of how the data were derived and so on. 3. Concluding remarksWe plan to continue filling in the database and developing its service. Certainly, many good papers and related Internet resources were missed by us. Therefore, we shall be very thankful to anyone who could send us more references, data files, or links to be included in the database. Any comments and remarks are also welcome. Our contact address is vi2087@vi2087.spb.edu.Acknowledgements: The authors acknowledge the financial support of the Volkswagen Foundation (Germany) that made this work possible. References:
|
To the top