Mineral mapping on the Moon surface provides the clue to understand the origin, evolution, stratigraphy and geological history of the Moon. Recently, reflectance imaging spectroscopy plays a significant role in identifying minerals on the planetary surface in the Visible to NIR region of the electromagnetic spectrum. The Moon Mineralogy Mapper (M3) onboard Chandrayaan-1 provides unprecedented spectral data of lunar surface to study about the Moon surface. Here we used the M3 sensor data (hyperspectral imaging spectroscopy) for analysing mineralogy of Orientale basin region on the Moon surface. Reflectance spectrums were sampled from different locations of the basin and continuum was removed using ENvironment for Visualizing Images (ENVI) so...
These mineral maps are derived using Multiband Imager (MI_MAP_02) reflectance data and Hapke radiati...
This Dissertation comprises three distinct research projects, all of which employ the use of remote ...
Near-IR reflectance spectra (0.6-2.5 m) and CCD images in the extended visible range (0.4-1.0 m) obt...
Mineral mapping on the Moon surface provides the clue to understand the origin, evolution, stratigra...
Mineralogy of the Lunar surface provides important clues for understanding the composition and evolu...
AbstractMineralogy of the Lunar surface provides important clues for understanding the composition a...
The imaging spectroscopy offers an opportunity to map and discriminate different minerals on the lun...
Mare Ingenii is a site of great interest for lunar geology as it is one of the few basaltic plains o...
A positive identification of the minerals olivine, plagioclase, and several types of pyroxenes were ...
International audienceThe spectral analysis of a planetary surface is fundamental for a deeper under...
AbstractMineralogy of the Lunar surface provides important clues for understanding the composition a...
The major mineralogical components of Yamato-791197 determined from reflectance spectra are calcium-...
International audienceThe spectral analysis of a planetary surface is fundamental for a deeper under...
The visible and near-infrared imaging spectrometer on board the Yutu Rover of Chinese Chang'E-3 ...
Analysis of lunar samples returned by the US Apollo missions revealed that the lunar highlands consi...
These mineral maps are derived using Multiband Imager (MI_MAP_02) reflectance data and Hapke radiati...
This Dissertation comprises three distinct research projects, all of which employ the use of remote ...
Near-IR reflectance spectra (0.6-2.5 m) and CCD images in the extended visible range (0.4-1.0 m) obt...
Mineral mapping on the Moon surface provides the clue to understand the origin, evolution, stratigra...
Mineralogy of the Lunar surface provides important clues for understanding the composition and evolu...
AbstractMineralogy of the Lunar surface provides important clues for understanding the composition a...
The imaging spectroscopy offers an opportunity to map and discriminate different minerals on the lun...
Mare Ingenii is a site of great interest for lunar geology as it is one of the few basaltic plains o...
A positive identification of the minerals olivine, plagioclase, and several types of pyroxenes were ...
International audienceThe spectral analysis of a planetary surface is fundamental for a deeper under...
AbstractMineralogy of the Lunar surface provides important clues for understanding the composition a...
The major mineralogical components of Yamato-791197 determined from reflectance spectra are calcium-...
International audienceThe spectral analysis of a planetary surface is fundamental for a deeper under...
The visible and near-infrared imaging spectrometer on board the Yutu Rover of Chinese Chang'E-3 ...
Analysis of lunar samples returned by the US Apollo missions revealed that the lunar highlands consi...
These mineral maps are derived using Multiband Imager (MI_MAP_02) reflectance data and Hapke radiati...
This Dissertation comprises three distinct research projects, all of which employ the use of remote ...
Near-IR reflectance spectra (0.6-2.5 m) and CCD images in the extended visible range (0.4-1.0 m) obt...