International audienceWe use laboratory experiments and radiative transfer modeling to study how the 1.9- and 3-μm H2O absorption bands are affected by variations of mineral particle size and albedo. A consistency between results of physical experiments and numerical simulations demonstrates that the studied effects are well described by the theory of radiative transfer in particulate media. Band strengths show different relationships with particle size, depending on the absolute intensity of the absorption and the criterion used to calculate band strength (band depth, area, ESPAT function, etc.). Various mixing processes used to vary sample albedo reveal a strong dependence of band strengths with albedo. For the 1.9-μm band, those effects ...
Interlayer cations and moisture content greatly influence the molecular vibrations of H2O in montmor...
Fourier transform infrared (FTIR) spectroscopy can be used to determine the concentration and speci...
The surface morphology of most of the airless planetary objects is characterized by the covering of ...
International audienceWe use laboratory experiments and radiative transfer modeling to study how the...
International audienceQuantitative effects of incidence and emergence angles variations on the 1.9- ...
Near-IR reflectance spectroscopy is widely used to detect mineral hydration on Solar System surfaces...
[1] Fundamental and overtone vibrational absorptions of H2O and OH observed in reflectance spectra ...
International audienceWe analyze the origins of the 3 µm water-of-hydration band strength spatial va...
International audienceWe use laboratory experiments and radiative transfer modeling to determine the...
Reflectance spectra were computed for water ice and ammonia ice mixtures as functions of weight frac...
Using IR absorption data from polarized measurements on single-crystal minerals with stoichiometric ...
The Solar light reflected by the Martian surface in the spectral range of near infrared reveals the ...
Real planetary surfaces are composed of several to many different minerals and ices. Deconvolving a ...
We examined the light-absorption properties of various samples of mineral particles suspended in wat...
This study focuses on particle size effect on monomineralic powders recorded using attenuated total ...
Interlayer cations and moisture content greatly influence the molecular vibrations of H2O in montmor...
Fourier transform infrared (FTIR) spectroscopy can be used to determine the concentration and speci...
The surface morphology of most of the airless planetary objects is characterized by the covering of ...
International audienceWe use laboratory experiments and radiative transfer modeling to study how the...
International audienceQuantitative effects of incidence and emergence angles variations on the 1.9- ...
Near-IR reflectance spectroscopy is widely used to detect mineral hydration on Solar System surfaces...
[1] Fundamental and overtone vibrational absorptions of H2O and OH observed in reflectance spectra ...
International audienceWe analyze the origins of the 3 µm water-of-hydration band strength spatial va...
International audienceWe use laboratory experiments and radiative transfer modeling to determine the...
Reflectance spectra were computed for water ice and ammonia ice mixtures as functions of weight frac...
Using IR absorption data from polarized measurements on single-crystal minerals with stoichiometric ...
The Solar light reflected by the Martian surface in the spectral range of near infrared reveals the ...
Real planetary surfaces are composed of several to many different minerals and ices. Deconvolving a ...
We examined the light-absorption properties of various samples of mineral particles suspended in wat...
This study focuses on particle size effect on monomineralic powders recorded using attenuated total ...
Interlayer cations and moisture content greatly influence the molecular vibrations of H2O in montmor...
Fourier transform infrared (FTIR) spectroscopy can be used to determine the concentration and speci...
The surface morphology of most of the airless planetary objects is characterized by the covering of ...