The Cassini Synthetic Aperture Radar (SAR) has been acquiring images of Titan's surface since October 2004. Radar data suffer from speckle noise hindering interpretation of small-scale features and comparison of reimaged regions for topography derivation and potential detection. By combining a state of the art denoising algorithm with mapping and quantitative measurements we greatly offer previously unattainable insights and introducing the denoising version of the Cassini SAR named NLDSAR.