Add to ORKGVEM-window data are shown to distinguish among key rock types on Venus, and evaluate redox state and transition metal contents of Venus surface rocks
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
New high-temperature emissivity measurements can provide important insights into the evolution of Ve...
The Venus Express mission has shown that orbital observations through transparent windows in the CO2...
In situ information on the surface composition of Venus is based on measurements of a small number o...
Interpretation of mineralogy using VNIR spectroscopy data from orbiters requires spectral libraries ...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
Machine learning models enable interpretation of orbital spectral measurements of Venus using labora...
The Venus Emissivity Mapper is the first flight instrument designed to focus on mapping the surface ...
Surface mineralogy records the primary composition, climate history and the geochemical cycling betw...
New observations from the Venus Express spacecraft as well as theoretical and experimental investiga...
New high-temperature emissivity measurements can provide important insights into the evolution of Ve...
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
New high-temperature emissivity measurements can provide important insights into the evolution of Ve...
The Venus Express mission has shown that orbital observations through transparent windows in the CO2...
In situ information on the surface composition of Venus is based on measurements of a small number o...
Interpretation of mineralogy using VNIR spectroscopy data from orbiters requires spectral libraries ...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
International audienceEmissivity data from ca. 1 micron lab measurements at DLR demonstrate the abil...
Machine learning models enable interpretation of orbital spectral measurements of Venus using labora...
The Venus Emissivity Mapper is the first flight instrument designed to focus on mapping the surface ...
Surface mineralogy records the primary composition, climate history and the geochemical cycling betw...
New observations from the Venus Express spacecraft as well as theoretical and experimental investiga...
New high-temperature emissivity measurements can provide important insights into the evolution of Ve...
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
Using five band orbital emissivity measurements in the 1 micron region has tremendous potential to p...
New high-temperature emissivity measurements can provide important insights into the evolution of Ve...