Two lunar soils: basalt and anorthosite, three glasses: synthetic glass, basalt glass, and obsidian measured in emissivity at 140°C. Soil with 20 µm glass on top was measured too, then heated to 900°C for four hours and then again measured in emissivity
In October 2020, BepiColombo performed a flyby maneuver at the Moon. The Mercury Radiometer and Ther...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
The BepiColombo mission is a joint project of the European Space Agency (ESA) and the Japan Aerospac...
The lunar infrared spectra (7-14 um) acquired by MERTIS on 10th April 2020 exhibit an unexpected max...
Presented here are infrared reflectance spectra of a typical set of Apollo samples to illustrate spe...
Here we present new laboratory spectral measurements of the major silicate minerals identified on th...
Currently, few thermal infrared measurements exist of fine particulate ( < 63 μm) analogue samples (...
To facilitate the development of the MERTIS instrument for BepiColombo, a list of Mercury analogue m...
Here we present a comprehensive set of laboratory measurements from the ultraviolet (UV) to the far...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements i...
Introduction: The mid infrared (MIR) spectral region is especially sensitive to the abundance of Si-...
Lunar sample measurements were made both under ambient nitrogen pressure and under vacuum conditions...
We present results of spectral unmixing analyses of labradorite-enstatite-glass mineral mixtures usi...
The unmixing model used in this study has previ- ously been used for spectral unmixing of NASA RELAB...
In October 2020, BepiColombo performed a flyby maneuver at the Moon. The Mercury Radiometer and Ther...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
The BepiColombo mission is a joint project of the European Space Agency (ESA) and the Japan Aerospac...
The lunar infrared spectra (7-14 um) acquired by MERTIS on 10th April 2020 exhibit an unexpected max...
Presented here are infrared reflectance spectra of a typical set of Apollo samples to illustrate spe...
Here we present new laboratory spectral measurements of the major silicate minerals identified on th...
Currently, few thermal infrared measurements exist of fine particulate ( < 63 μm) analogue samples (...
To facilitate the development of the MERTIS instrument for BepiColombo, a list of Mercury analogue m...
Here we present a comprehensive set of laboratory measurements from the ultraviolet (UV) to the far...
One of the key problems in determining lunar surface composition for thermal-infrared measurements ...
One of the key problems in determining lunar surface composition for thermal-infrared measurements i...
Introduction: The mid infrared (MIR) spectral region is especially sensitive to the abundance of Si-...
Lunar sample measurements were made both under ambient nitrogen pressure and under vacuum conditions...
We present results of spectral unmixing analyses of labradorite-enstatite-glass mineral mixtures usi...
The unmixing model used in this study has previ- ously been used for spectral unmixing of NASA RELAB...
In October 2020, BepiColombo performed a flyby maneuver at the Moon. The Mercury Radiometer and Ther...
Remote-sensing infrared spectroscopy is the principal field of investigation for planetary surfaces ...
The BepiColombo mission is a joint project of the European Space Agency (ESA) and the Japan Aerospac...