2. Characterization of the Martian surface using an index

As shown by figure 11b and 11d , as the collimator aperture position is in front of the center of a pixel column, the whole pseudo-pixel surface is reconstructed: no difference

Firstly, images in degree of polarization can differentiate much better the bonding points from the fibrous background than intensity images (Fig. Moreover, the

Indeed, these two ideas are combined in the instrument through a lenslet array: the interferometric slides has step case shape, so that in front of each microlens there is a

Here, we apply these spectral criteria to reflectance spectra of terrestrial opals and to CRISM data in order to evaluate their validity on Martian data and to better

Le comportement est certainement influencé par les dimensions géométriques des éléments structuraux (Le voile et la semelle) notamment la hauteur, l’épaisseur, les longueurs

representations theory, we classify their irreducible unitary representations, and study the neighborhood of the trivial representation (which is closely connected to

OMEGA observations reveal that the albedo and spectral evolution during spring and summer results from a wide range of processes, involving changes in effective grain size of the CO

Right panel: density profile of the cloud (image m) and the first eleven Bogoliubov modes for a gas at rest in the final trap. Comparison of the first principal components oscil-