Laboratory measurements were performed to study the spectral signature of H2O ice between 0.4 and 4.2 µm depending on varying temperatures between 70 and 220 K. Spectral parameters of samples with particle sizes up to ~1360 µm, particle size mixtures, and different particle shapes were analyzed. The band depth (BD) of the major H2O-ice absorptions at 1.04, 1.25, 1.5, and 2 µm offers an excellent indicator for varying particle sizes in pure H2O ice. The spectral changes due to temperature rather, but not exclusively, affect the H2O-ice absorptions located at 1.31, 1.57, and 1.65 µm and the Fresnel reflection peaks at 3.1 and 3.2 µm, which strongly weaken with increasing temperature. As the BDs of the H2O-ice absorptions at 1.31, 1.57, and 1....
The relative abundances of ices in astrophysical environments rely on accurate laboratory measuremen...
Magnetospheric radiation drives surface and near-surface chemistry on Europa, but below a few meters...
Infrared detection of water ice phase can reveal the temperature and radiation history of a surface....
International audienceLaboratory measurements were performed to study the spectral signature of H2O ...
The detailed investigation of the variations in the H2O-ice spectral signatures across Ganymede's an...
Three satellites of Jupiter, seven satellites of Saturn, and five satellites of Uranus show spectros...
In this paper we present spectra of H2O2-containing ices in the near- and mid-infrared (IR) regions....
Context. Recent mid-infrared spectroscopic observations of Pluto and Triton suggest a wide distribut...
Interstellar ices are largely composed of frozen water. It is important to derive fundamental parame...
Visual-to-infrared (VIS-IR) remote sensing observations of different classes of outer solar system o...
Using new laboratory spectra, we have calculated the real and imaginary parts of the index of refrac...
Laboratory spectra have shown that CO2 is a powerful diagnostic tool for analyzing infrared data fro...
The optical properties of ice in the far infrared are important for models of protoplanetary and deb...
The techniques of low temperature spectroscopy are applied to identify the constituents of the ices ...
Context. New spectroscopic observations in the far-infrared (IR) range are expected from future plan...
The relative abundances of ices in astrophysical environments rely on accurate laboratory measuremen...
Magnetospheric radiation drives surface and near-surface chemistry on Europa, but below a few meters...
Infrared detection of water ice phase can reveal the temperature and radiation history of a surface....
International audienceLaboratory measurements were performed to study the spectral signature of H2O ...
The detailed investigation of the variations in the H2O-ice spectral signatures across Ganymede's an...
Three satellites of Jupiter, seven satellites of Saturn, and five satellites of Uranus show spectros...
In this paper we present spectra of H2O2-containing ices in the near- and mid-infrared (IR) regions....
Context. Recent mid-infrared spectroscopic observations of Pluto and Triton suggest a wide distribut...
Interstellar ices are largely composed of frozen water. It is important to derive fundamental parame...
Visual-to-infrared (VIS-IR) remote sensing observations of different classes of outer solar system o...
Using new laboratory spectra, we have calculated the real and imaginary parts of the index of refrac...
Laboratory spectra have shown that CO2 is a powerful diagnostic tool for analyzing infrared data fro...
The optical properties of ice in the far infrared are important for models of protoplanetary and deb...
The techniques of low temperature spectroscopy are applied to identify the constituents of the ices ...
Context. New spectroscopic observations in the far-infrared (IR) range are expected from future plan...
The relative abundances of ices in astrophysical environments rely on accurate laboratory measuremen...
Magnetospheric radiation drives surface and near-surface chemistry on Europa, but below a few meters...
Infrared detection of water ice phase can reveal the temperature and radiation history of a surface....