Topographic modeling of Phoebe using Cassini images
22 août 2006 High-resolution Cassini stereo images of Saturn's moon Phoebe have been used to derive a regional digital terrain model (DTM) and.
Determining a tilt in Titan's north–south albedo asymmetry from
Analysis of Titan's hemispheric brightness asymmetry from mapped Cassini images reveals an axis of symmetry that is tilted with respect to the rotational
Vertical wind shear on Jupiter from Cassini images
[1] Multifilter images of Jupiter acquired by the Cassini Imaging Science Subsystem vertical wind shear by tracking clouds in images at different.
Saturn eddy momentum fluxes and convection: First estimates from
Voyager Saturn manually tracked images had suggested no conversion Images were flux calibrated using Cassini Imaging Sci-.
Edge detection in Cassini astronomy image using Extreme Learning
proposed for Cassini astronomy images. In the ELM model a 28-D feature vector of a pixel in Cassini image is constructed as input
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Life cycles of spots on Jupiter from Cassini images
Life cycles of spots on Jupiter from Cassini images. Liming Lia∗.
Edge detection applied to Cassini images reveals no measurable
18 juil. 2012 Edge detection applied to Cassini images reveals no measurable displacement of Ontario Lacus' margin between 2005 and 2010.
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Focus sur le pendule de Huygens
A en croire la légende c'est en observant les oscillations du lustre de la cathédrale de. Pise en 1581 que le jeune Galilée découvrit que l'amplitude des
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Multilayer hazes over Saturn's hexagon from Cassini ISS limb images
In June 2015 Cassini high-resolution images of Saturn's limb southwards of the planet's hexagonal wave revealed a system of at least six stacked haze
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Saturn eddy momentum fluxes and convection: First estimates from
Voyager Saturn manually tracked images had suggested no conversion Images were flux calibrated using Cassini Imaging Sci-.