© 2020 Elsevier Ltd The focus of this paper is to study the application of the first order derivative method for the estimation of minerals rates in different mineral mixtures. The primary goal with this is to find robust spectral features of specific minerals that are not severely influenced by the spectral features of the other minerals in a mixture. Results were used to select appropriate spectral features to be applied for quantifying the minerals in upcoming studies. Mixtures of different terrestrial minerals equivalent to those dominating the Martian surface with a grain size \u3c0.25 mm were prepared and analyzed in the laboratory by reflectance spectroscopy in the VNIR-SWIR range. The first derivatives were computed and correlated ...
The imaging spectroscopy offers an opportunity to map and discriminate different minerals on the lun...
A positive identification of the minerals olivine, plagioclase, and several types of pyroxenes were ...
The lunar surface consists of a regolith layer that covers the underlying bedrocks, and is generally...
© 2020 Elsevier Ltd The focus of this paper is to study the application of the first order derivativ...
International audienceThe behavior of the three primary olivine absorptions near 1 μm (referred to a...
We present results of spectral unmixing analyses of labradorite-enstatite-glass mineral mixtures usi...
Among the techniques to detect planet's mineralogical composition remote sensing, visible and near-i...
The unmixing model used in this study has previ- ously been used for spectral unmixing of NASA RELAB...
The reflectance spectra of combinations of olivine, orthopyroxene, and iron meteorite metal show sys...
Abstract. Reflectance spectra of olivines spanning the forsterite-fayalite solid-solution series hav...
AbstractIron-bearing minerals are a major component of planetary surfaces, and many can be identifie...
The Mare Moscoviense is an astonishing rare flatland multi-ring basin and one of the recognizable ma...
We examined the influence of micrometeorite bombardment simulated with an excimer laser, which irrad...
We proposed a model to determine the spectral reflectance of mineral mixtures as a function of relat...
Among the Solar System’s bodies, Moon, Mercury and Mars are at present, or have been in the recent y...
The imaging spectroscopy offers an opportunity to map and discriminate different minerals on the lun...
A positive identification of the minerals olivine, plagioclase, and several types of pyroxenes were ...
The lunar surface consists of a regolith layer that covers the underlying bedrocks, and is generally...
© 2020 Elsevier Ltd The focus of this paper is to study the application of the first order derivativ...
International audienceThe behavior of the three primary olivine absorptions near 1 μm (referred to a...
We present results of spectral unmixing analyses of labradorite-enstatite-glass mineral mixtures usi...
Among the techniques to detect planet's mineralogical composition remote sensing, visible and near-i...
The unmixing model used in this study has previ- ously been used for spectral unmixing of NASA RELAB...
The reflectance spectra of combinations of olivine, orthopyroxene, and iron meteorite metal show sys...
Abstract. Reflectance spectra of olivines spanning the forsterite-fayalite solid-solution series hav...
AbstractIron-bearing minerals are a major component of planetary surfaces, and many can be identifie...
The Mare Moscoviense is an astonishing rare flatland multi-ring basin and one of the recognizable ma...
We examined the influence of micrometeorite bombardment simulated with an excimer laser, which irrad...
We proposed a model to determine the spectral reflectance of mineral mixtures as a function of relat...
Among the Solar System’s bodies, Moon, Mercury and Mars are at present, or have been in the recent y...
The imaging spectroscopy offers an opportunity to map and discriminate different minerals on the lun...
A positive identification of the minerals olivine, plagioclase, and several types of pyroxenes were ...
The lunar surface consists of a regolith layer that covers the underlying bedrocks, and is generally...