During 10 years of discovery, NASA’s Cassini spacecraft has pulled back the smoggy veil that obscures the surface of Titan, Saturn’s largest moon. Cassini’s radar instrument has mapped almost half of the giant moon’s surface; revealed vast, desert-like expanses of sand dunes; and plumbed the depths of expansive hydrocarbon seas. What could make that scientific bounty even more amazing? Well, what if the radar images could look even better?
Thanks to a recently developed technique for handling noise in Cassini’s radar images, these views now have a whole new look. The technique, referred to by its developers as “despeckling,” produces images of Titan’s surface that are much clearer and easier to look at than the views to which scientists and the public have grown accustomed.
Typically, Cassini’s radar images have a characteristic grainy appearance. This “speckle noise” can make it difficult for scientists to interpret small-scale features or identify changes in images of the same area taken at different times.
Despeckling uses an algorithm to modify the noise, resulting in clearer views that can be easier for researchers to interpret.
Antoine Lucas got the idea to apply this new technique while working with members of Cassini’s radar team when he was a postdoctoral researcher at the California Institute of Technology in Pasadena.
Presented here are side-by-side comparisons of a traditional Cassini Synthetic Aperture Radar (SAR) view and one made using a new technique for handling electronic noise that results in clearer views of Titan’s surface. Image credit: NASA/JPL-Caltech/ASI.