Database of Optical Constants for Cosmic Dust

Laboratory Astrophysics Group of the AIU Jena


Note: Users of these data are kindly asked to cite the original papers. Links to the literature can be found in the header of each class of materials. Thank you. H.M. 23/08/06

THIS WEB SITE HAS BEEN MOVED. Links may not work. Please proceed to: https://www.astro.uni-jena.de/Laboratory/OCDB/index.html. Thank you. H.M. 08/04/21

Selection
   

Optical Constants of Oxides and Sulfides:

Magnesium-iron sulfides: (Begemann et al. 1994)
Mg0.9Fe0.1S
Spectran-k-Data

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Mg0.75Fe0.25S
Spectran-k-Data

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Mg0.5Fe0.5 S
Spectran-k-Data

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Mg0.1Fe0.9 S
Spectran-k-Data

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Fe S
Spectran-k-Data

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Magnesium-iron oxides: (Henning et al. 1995)
Mg0.6 Fe0.4 O [4.79 g/ccm]
Spectran-k-Data

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Mg0.5 Fe0.5 O
Spectran-k-Data

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Mg0.3 Fe0.7 O [5.05 g/ccm]
Spectran-k-Data

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Mg0.2 Fe0.8 O [5.25 g/ccm]
Spectran-k-Data

<>Link to a 300dpi and a 600dpi image
 

Mg0.1 Fe0.9 O [5.46 g/ccm]
Spectran-k-Data

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FeO [5.70 g/ccm]
Spectran-k-Data

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Iron oxides, created by Amaury H.M.J. Triaud, (Amaury.Triaud@obs.unige.ch) unpublished:
Fe3 O4
Spectran-k-Data

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Fe2 O3, E || a,b
Spectran-k-Data

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Silicon disulfide: (Begemann et al. 1996)
Si S2
Spectran-k-Data

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Aluminum oxide (amorphous): (Begemann et al. 1997)
Al2 O3 (porous)
Spectran-k-Data

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Al2 O3 (compact)
Spectran-k-Data

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Natural and natural-thermal-processed Mg-spinels (crystalline) (Fabian et al. 2001)
MgAl2 O4 (natural)
Spectran-k-Data

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MgAl2 O4 (natural, annealed 1h, 1223 K)
Spectran-k-Data

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Additional information
about this natural spinel and the thermal processing
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Nonstoichiometric Mg-spinels (crystalline): (Fabian et al. 2001)
Mg1.01 Al1.99 O4 (synthetic)
Spectran-k-Data

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Mg0.94 Al2.04 O4 (synthetic)
Spectran-k-Data

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Mg0.82 Al2.12 O4 (synthetic)
Spectran-k-Data

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Mg0.73 Al2.17 O4 (synthetic)
Spectran-k-Data

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Mg0.53 Al2.31 O4 (synthetic)
Spectran-k-Data

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Mg0.43 Al2.38 O4 (synthetic)
Spectran-k-Data

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Additional information
concerning the production and properties of these nonstoichiometric spinel
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Mg-spinels with impurities (crystalline) - NIR data: (Zeidler et al. 2011)
Mg1.02 Al1.93 Cr0.0087 Fe0.012 O4 (natural, Burma)
Spectran-k-Data

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Mg1.00 Al1.98 Cr0.02 O4 (synthetic)
Spectran-k-Data

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Mg0.93 Al1.99 Cr0.03 O4 (synthetic)
Spectran-k-Data

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Mg0.98 Al1.89 Cr0.12 O4 (synthetic)
Spectran-k-Data

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Mg0.98 Al1.78 Cr0.23 O4 (synthetic)
Spectran-k-Data

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Hibonite (CaAl12O19): (Mutschke et al. 2002)
Spectra

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Hibonite E || c n-k-Data
 
Hibonite E || a,b n-k-Data
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Titanium oxides: (Posch et al. 2003, Zeidler et al. 2011)
TiO2 (Rutile, ord. ray)
Spectra

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Rutile E || a,b n-k-Data

TiO2 (Rutile, extraord. ray)
Spectra

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Rutile E || c n-k-Data

TiO2 (Anatase)
Spectra

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Anatase E || c n-k-Data
Anatase E || a,b n-k-Data

TiO2 (Anatase) NIR absorption
Spectra

Link to a 300dpi and a 600dpi image
k-Data

TiO2 (Brookite)
Spectra

Link to a 300dpi and a 600dpi image
Brookite E || x n-k-Data
Brookite E || y n-k-Data
Brookite E ||z n-k-Data

CaTiO3 (Perovskite)
Spectran-k-Data

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All n-k-Data tables consist of three columns. The first one contains the wavelength in micron (in the case of the Mg/Fe sulfides centimeter). The second one is the real part of the complex refractive index (n), the third one is the imaginary part (k). Values in brackets given after the chemical formulae are the material densities (if available).


For the details of the derivation of all n-k-Data I refer to the mentioned publications (see the List of Publications).


Optical Database main page Laboratory main page Institute home page

First design: Harald Mutschke, September 2002
Images created by Hannes Richter (Sternwarte Wien)
New Design: Jürgen Weiprecht, October 2004 and new ideas from Thomas Posch in Februar/March 2005
Last modified: 06.03.2005, 07-17.03.2005 Malte Meinecke, Benedikt Pfrimmer
Content checked: Harald Mutschke, 18.04.2005
Last modified: 20.02.2020 JW