The Berlin emissivity database is a spectral library providing a basis for the interpretation of thermal emission spectra of planetary regoliths. It contains spectra of plagioclase and potassium feldspars, low and high Ca pyroxenes, olivine, sulfur, Martian analogs, and a lunar highland sample in the wavelength range 3-50 μm. Four particle sizes with dimensions <25, 25-63, 63-125, 125-250 μm are measured for each sample. An exhaustive suite of tests was implemented, to characterize the setup in the planetary emissivity laboratory and the emissivities collected in the spectral library. The tests improve the quality of measurements, optimizing the sample preparation, calibration algorithm, sample, blackbody, and chamber temperatures, and all ...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
The Berlin Reflectance Spectral Library (BRSL) provides a collection of reflectance spectra between ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
Mineralogical composition study of planetary surfaces is mostly performed by means of remote sensing...
The Berlin Emissivity Database contains spectra of feldspars, pyroxenes, olivine, sulphur, martian a...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
<p>Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfac...
Spectral Library: The Berlin Emissivity Database (BED) is a spectral library containing the emissi...
The Planetary Fourier Spectrometer (PFS) onboard the Mars Express Mission provides thermal infrared,...
In the last decade several IR spectrometers flew on spacecrafts around terrestrial planets (e.g. PFS...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
Spectroscopy is still the most accurate methodology to study the surface composition (and its evolut...
[1] New laboratory thermal infrared emissivity measurements of the plagioclase solid solution serie...
We have measured the emissivity and reflectance spectra for a suite of analogues of relevance for as...
At the Planetary Emissivity Laboratory (PEL) of the German Aerospace Center, DLR, in Berlin we are ...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
The Berlin Reflectance Spectral Library (BRSL) provides a collection of reflectance spectra between ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
Mineralogical composition study of planetary surfaces is mostly performed by means of remote sensing...
The Berlin Emissivity Database contains spectra of feldspars, pyroxenes, olivine, sulphur, martian a...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
<p>Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfac...
Spectral Library: The Berlin Emissivity Database (BED) is a spectral library containing the emissi...
The Planetary Fourier Spectrometer (PFS) onboard the Mars Express Mission provides thermal infrared,...
In the last decade several IR spectrometers flew on spacecrafts around terrestrial planets (e.g. PFS...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
Spectroscopy is still the most accurate methodology to study the surface composition (and its evolut...
[1] New laboratory thermal infrared emissivity measurements of the plagioclase solid solution serie...
We have measured the emissivity and reflectance spectra for a suite of analogues of relevance for as...
At the Planetary Emissivity Laboratory (PEL) of the German Aerospace Center, DLR, in Berlin we are ...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
The Berlin Reflectance Spectral Library (BRSL) provides a collection of reflectance spectra between ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...