NASA, JAXA and ESA plan to send sample return missions to asteroids. At PEL we measured emissivity of meteorites, sulfates, carbonates, phyllos as analogs
Phyllosilicates on Mars have been identified few years ago by the OMEGA instrument on the ESA Mars E...
Dependence of laboratory-measured emissivity spectra from the emergence angle is a subject that stil...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
Space missions to asteroids are becoming more and more common. Appropriate spectroscopic measurement...
We have measured the emissivity and reflectance spectra for a suite of analogues of relevance for as...
At the Planetary Emissivity Laboratory (PEL) of DLR in Berlin we set-up an experiment to measure the...
At the Planetary Emissivity Laboratory (PEL) of the German Aerospace Center, DLR, in Berlin we are ...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
Reflectance (Tsample=20°C) and emissivity (Tsample=100°C) for 10 analogues measured in vacuum in 1-...
We describe the capabilities, radiometric stability, and calibration of a custom vacuum environment ...
We studied the influence of emerging angle on emissivity spectra measured in air and in vacuum, with...
Mineralogical composition study of planetary surfaces is mostly performed by means of remote sensing...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
The Berlin Emissivity Database contains spectra of feldspars, pyroxenes, olivine, sulphur, martian a...
Phyllosilicates on Mars have been identified few years ago by the OMEGA instrument on the ESA Mars E...
Dependence of laboratory-measured emissivity spectra from the emergence angle is a subject that stil...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
Space missions to asteroids are becoming more and more common. Appropriate spectroscopic measurement...
We have measured the emissivity and reflectance spectra for a suite of analogues of relevance for as...
At the Planetary Emissivity Laboratory (PEL) of DLR in Berlin we set-up an experiment to measure the...
At the Planetary Emissivity Laboratory (PEL) of the German Aerospace Center, DLR, in Berlin we are ...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
The last decades have seen a large number of missions targeting small bodies in the solar system. NA...
Reflectance (Tsample=20°C) and emissivity (Tsample=100°C) for 10 analogues measured in vacuum in 1-...
We describe the capabilities, radiometric stability, and calibration of a custom vacuum environment ...
We studied the influence of emerging angle on emissivity spectra measured in air and in vacuum, with...
Mineralogical composition study of planetary surfaces is mostly performed by means of remote sensing...
The Institute for Planetary Research has an expertise in spectroscopy of minerals, rocks, meteorites...
The Berlin Emissivity Database contains spectra of feldspars, pyroxenes, olivine, sulphur, martian a...
Phyllosilicates on Mars have been identified few years ago by the OMEGA instrument on the ESA Mars E...
Dependence of laboratory-measured emissivity spectra from the emergence angle is a subject that stil...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...