This study presents a 13 years survey of haze UV extinction profiles, monitoring the temporal evolution of the detached haze layer (DHL) in Titan's upper atmosphere (350-600 km). As reported by West et al. 2011 (GRL vol.38, L06204) at the equator, we show that the DHL is present at all latitudes below 55°N during the northern winter (2004-2009)....

Titan global map merging VIMS and ISS datasets, details were presented by B. Seignovert et al. at LPSC 2019 and EPSC/DPS 2019 (cf. related identifiers).

This data set is a g-zipped, tarred collection of jpg mosaics projected above Jupiter's north pole for filters UV1 and MT3 (for a description of the filters see C. Porco et al., Space Science Reviews 115: 363–497, 2004. For a description of ISS activity for the Jupiter flyby see Porco et al., SCIENCE VOL 299 7 MARCH 2003, page 1541.

This file is a movie of Jupiter's northern hemisphere during the Cassini approach, October - December, 2000. It is composed of a time sequence of frames in the UV1 filter, effective wavelength 258 nm. Each frame is a mosaic from six or more images mapped to a projection with the north pole at the center and the radial distance proportional to ...