Optical n-k-Data

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. Litxts to the literature can be found in the header of each class of materials. Thatxt you. H.M. 23/08/06

Selection
   

Optical Constants of Carbonates

Calcite (CaCO3) (Posch et al. 2007)
CaCO3 (10 K)
Spectra

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

CaCO3 (100 K)
Spectra

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

CaCO3 (200 K)
Spectra

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

CaCO3 (300 K)
Spectra

Litxt to a 300dpi and a 600dpi image
Calcite E || c n-k-Data
Calcite E || a,b n-k-Data
Top Optical Database main page
Dolomite (CaMg(CO3)2) (Posch et al. 2007)
CaMg(CO3)2 (10 K)
Spectra

Litxt 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

Litxt 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

Litxt 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

Litxt to a 300dpi and a 600dpi image
Dolomite E || c n-k-Data
Dolomite E || a,b n-k-Data
 
Top Optical Database main page

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

Design: Jürgen Weiprecht, Thomas Posch, Malte Meinecke, Benedikt Pfrimmer, Harald Mutschke
Responsible for Data: Harald Mutschke
Images created by Hannes Richter (Sternwarte Wien)
Last edit: 24.02.2020 JW