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

Selection
   

Optical Constants at low Temperatures

The optical constants have been determined by Kramers-Kronig analysis from reflectance measurements at polished surfaces of bulk samples. Experimental details are given in Henning and Mutschke (1997), Posch et al. (2007) :

Amorphous SiO2 (quartz glass):
SiO2 (10K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 

SiO2 (100K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 

SiO2 (200K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 

SiO2 (300K)
Spectran-k-Data

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amorphous pyroxene of "cosmic" composition
pyroxene (10K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

pyroxene (100K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

pyroxene (200K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

pyroxene (300K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 
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crystalline pyroxene (bronzite)
Bronzite (10K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

Bronzite (100K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

Bronzite (200K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

Bronzite (300K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 
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iron oxide (FeO)
FeO (10 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeO (100 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeO (200 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeO (300 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
 
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iron sulfide (FeS)
FeS (10 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeS (100 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeS (200 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image

FeS (300 K)
Spectran-k-Data

Link to a 300dpi and a 600dpi image
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Calcite (CaCO3)
CaCO3 (10 K)
Spectra

Link to a 300dpi and a 600dpi image
Calcite E || c n-k-Data
Calcite E || a,b n-k-Data

CaCO3 (100 K)
Spectra

Link to a 300dpi and a 600dpi image
Calcite E || c n-k-Data
Calcite E || a,b n-k-Data

CaCO3 (200 K)
Spectra

Link to a 300dpi and a 600dpi image
Calcite E || c n-k-Data
Calcite E || a,b n-k-Data

CaCO3 (300 K)
Spectra

Link to a 300dpi and a 600dpi image
Calcite E || c n-k-Data
Calcite E || a,b n-k-Data
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Dolomite (CaMg(CO3)2)
CaMg(CO3)2 (10 K)
Spectra

Link to a 300dpi and a 600dpi image
Dolomite E || c n-k-Data
Dolomite E || a,b n-k-Data

CaMg(CO3)2 (100 K)
Spectra

Link to a 300dpi and a 600dpi image
Dolomite E || c n-k-Data
Dolomite E || a,b n-k-Data

CaMg(CO3)2 (200 K)
Spectra

Link to a 300dpi and a 600dpi image
Dolomite E || c n-k-Data
Dolomite E || a,b n-k-Data

CaMg(CO3)2 (300 K)
Spectra

Link to a 300dpi and a 600dpi image
Dolomite E || c n-k-Data
Dolomite E || a,b n-k-Data
 
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All n-k-Data tables consist of three columns. The first one contains the wavelength in micron. The second one is the real part of the complex refractive index (n), the third one is the imaginary part (k).


For the details of the derivation of all n-k-Data we 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: 20.04.2005 JW